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Exploring protostellar disk formation via misaligned rotation axes and magnetic field, and their observable features. The streamlines on the column density maps show the direction of flows along the picture frame. The black lines over Stokes Q and U parameters depict the direction of magnetic field estimated from the polarization angles. We predict that we witness magnetically directed spiraling behavior by polarization observations (Väisälä et al. 2019).
Observational signatures of early disk formation by MHD models
Figure shows an example of a nested-grid mesh refinement (NMR) run carried out by the Antares code for a global protoplanetary disk with an embedded circumplanetary disk surrounding a 0.05-Jupiter-mass planet at 5.2 AU from the star at origin. The simulation has 6 levels of refinement, with the finest resolution of 6.25×10–4 AU, resolving the Hill radius of the planet (0.13 AU at 5.2 AU) with ~200 cells. (Antares code with the CompAS project)
Formation and Evolution of Protoplanetary and Circumplanetary Disks with Antares Three-Dimensional Global Hydrodynamic Simulations
The panel of two figures illustrate the synthetic gas column density and linear polarization component q along the line of sight, inclined 15 degrees from the midplane, for a very early disk forming from collapsing magnetic flow with the Perspective code developed by the CHARMS project. The early disk in the model shows a spiral-like shape, presumably created by the magnetic field aligned along the rotational plane of the original cloud, that is streaming into the central source. (Perspective code; CHARMS Project; Väisälä, Shang et al., 2018, in preparation)
An early disk in formation from collapsing magnetic flows
This figures illustrate density profiles in log scale from simulations of two-temperature model of outflows from a young stellar object. (Left) Mosaic of simulations demonstrating effects of varying temperature and degree of magnetization. Panel indices from (a) to (c) shows decreasing magnetic field strength, and (1) to (3) shows increasing wind temperature. The central axial jet is more collimated and the shell structure is narrowed when the magnetic force is relatively important. (Zeus-TW simulations in Wang et al. 2015)
A Two-temperature Model of Magnetized Protostellar Outflows
Micrometer-scale ion images of the cross-section of SaU 290 (CH3 chondrite), recorded by the NanoSIMS 50L at Academia Sinica. A ~10 pA Cs+ primary beam with a nominal spot size of 100 nm and rastered over 20 × 20 µm, to image the sample surface simultaneously in several ion species. A total of 160 (10 × 16 rows) individual images were recorded, and these were combined to create maps in a) 16O- and b) 18O-, as well as c) secondary electrons.
Micrometer-scale ion images of the cross-section of SaU 290
Left – Surface density distribution of a forming circumplanetary disk in a protoplanetary disk with the Antares three-dimensional global simulation. A planet of one-Jupiter mass is placed at (x,y) = (5.2,0) au. The color scale is stretched logarithmically. The level boundaries of the nested-grid mesh refinement are shown in white lines. Center – Temperature distribution of the disk obtained with the radiative transfer code Hyperion. The photon sources are the central 4500-K star and an accreting planet of ~1000 K at 5.2 au from the star. The circumplanetary dust is heated up to ~ 1000 K and produces thermal emission. Right – Monochromatic synthetic image corresponding to the 1-mm dust continuum imaging, obtained with Hyperion. The surface brightness is logarithmically stretched in units of MJy/arcsec2.
Dust Radiative Transfer on a Global Hydrodynamic Simulation of a Forming Circumplanetary Disk
Illustration of wind model (left) and attempts to reproduce the velocity pattern of the blue lobe of the I04166 jet (right). The upper part of the left illustration shows two pieces of spherical shell layers, whose velocities point purly in spherical-r directions. The lower part shows how they appear on a position-velocity diagram, where two tooth-like features is seen. Such features greatly resemble the observed velocity pattern in the right. In the upper-right panel we plot the observed CO J=2–1 and CO J=3–2 emissions with blue contours, and the green line segments are model predictions. The color scale in the lower-right panel shows the synthesized CO J=2–1 PV diagram from one of our MHD numerical simulations. The good agreement demonstrates the feasibility of the wind geometry model. The simulated data was convolved with a Gaussian beam of 420 AU FWHM before extracting the PV diagram to better mimic the observation result.
Ejection History of Protostellar Outflow IRAS 04166+2706
<b>Left</b> – Surface density distribution of a forming circumplanetary disk in a protoplanetary disk with the Antares three-dimensional global simulation. A planet of one-Jupiter mass is placed at (x,y) = (5.2,0) au. The color scale is stretched logarithmically. The level boundaries of the nested-grid mesh refinement are shown in white lines. <b>Center</b> – Temperature distribution of the disk obtained with the radiative transfer code Hyperion. The photon sources are the central 4500-K star and an accreting planet of ~1000 K at 5.2 au from the star. The circumplanetary dust is heated up to ~ 1000 K and produces thermal emission. <b>Right</b> – Monochromatic synthetic image corresponding to the 1-mm dust continuum imaging, obtained with Hyperion. The surface brightness is logarithmically stretched in units of MJy/arcsec<sup>2</sup>.
Dust Radiative Transfer on a Global Hydrodynamic Simulation of a Forming Circumplanetary Disk
Kinematic properties of velocity-decomposed [Ne III] λ3869 emission are shown in a position–velocity (pv) diagram (left panel), a spatial profile along the jet axis (central panel), and line profiles at specific spatial positions (right three panels). In the pv diagram, the decomposed high-velocity component (HVC) and low-velocity component (LVC) are shown by green and red contours, respectively. The yellow symbols represent the HVC velocity centroids and orange symbols represent the LVC velocity centroids. The spatial profile is shown on a logarithmic scale to accommodate the large contrast between the innermost 3'' emission and the outer knots.
The [Ne III] Jet of DG Tau and Its Ionization Scenarios
A sample picture based on the radiative transfer code Perspective exploring a very early stage disk formed within the MHD model of Li et al. (2014). The picture shows gas column density and linear polarization component q along the line of sight, inclined 15 degrees from the midplane. The early disk in the model shows a spiral-like shape, presumably created by the magnetic field aligned along the rotational plane of the original cloud. (Väisälä, Shang et al., a work in progress)
Polarization Calculation and Visualization from MHD Simulation Data
Figure: Example of a nested-grid mesh refinement (NMR) run of a global protoplanetary disk with an embedded circumplanetary disk surrounding a 0.05-Jupiter-mass planet at 5.2 AU from the star at origin. The simulation has 6 levels of refinement, with the finest resolution of 6.25×10–4 AU, resolving the Hill radius of the planet (0.13 AU at 5.2 AU) with ~200 cells.
Formation and Evolution of Protoplanetary and Circumplanetary Disks with Antares Three-Dimensional Global Hydrodynamic Simulations
Illustration of wind model (left) and attempts to reproduce the velocity pattern of the blue lobe of the I04166 jet (right). The upper part of the left illustration shows two pieces of spherical shell layers, whose velocities point purly in spherical-r directions. The lower part shows how they appear on a position-velocity diagram, where two tooth-like features is seen. Such features greatly resemble the observed velocity pattern in the right. In the upper-right panel we plot the observed CO J=2–1 and CO J=3–2 emissions with blue contours, and the green line segments are model predictions. The color scale in the lower-right panel shows the synthesized CO J=2–1 PV diagram from one of our MHD numerical simulations. The good agreement demonstrates the feasibility of the wind geometry model. The simulated data was convolved with a Gaussian beam of 420 AU FWHM before extracting the PV diagram to better mimic the observation result.
Ejection History of Protostellar Outflow IRAS 04166+2706
Density plots in log scale from simulations of two-temperature outflow model. (Left) Mosaic of simulations demonstrating effects of varying temperature and magnetization degree. Panel indices of (a) to (c) shows decreasing magnetic field strength, and (1) to (3) shows increasing wind temperature. The central axial jet is less collimated and the shell structure is widened when magnetic force is relatively unimportant. (Right) Comparisons that demonstrates the effect of poloidal magnetic field. The top panel is run with poloidal field and the lower without. Thick solid line is where wind mass fraction is 1%, and thick dashed line is where bulk velocities equal the ambient sound speed. The shell is mode corrugated in cases without poloidal field (Wang et al. 2015)
A Two-temperature Model of Magnetized Protostellar Outflows
Distribution of the logarithm of the mass density ρ and velocity field (unit vectors) on the equatorial plane, for Models I (left panel, non-rotating) and J (right, rotating) that include both ambipolar diffusion and (enhanced) Ohmic dissipation for magnetic decoupling at small radii. Again, both models show filamentary structures in the inner protostellar accretion flow driven by magnetic interchange instability.
Protostellar Accretion Flows Destabilized by Magnetic Flux Redistribution
<b>Effects of temperature and magnetization on molecular outflows:</b> the structure of the base of outflows at 1000 yr is shown with different physical conditions. Panels (a) to (c) shows the Alfvénic Mach number from 6, 30, to 90 [decreasing magnetic field strength]; and (1) to (3) shows the wind temperature from 10 K, 400 K, to 2000 K [increasing wind temperature]. These corresponds to different plasma beta parameter (β<sub>plasma</sub> ≣ 8πa<sup>2</sup>ρ/B<sup>2</sup>) from 0.001 to 46. The central axial jet is less collimated and the shell structure is widened when β<sub>plasma</sub> increases. In these cases, the poloidal magnetic field in the toroid is not included.
Two-Temperature Model for Magnetized Protostellar Outflows
Snapshots of rotationally supported disks formed by introduced Hall effect in the MHD calculations, at a representative time of 2 x 10<sup>12</sup> sec.<br> <b>Left:</b> the edge-on view of the case with rotational axis and magnetic axis being parallel. The poloidal velocity field is shown in white arrows and the magnetic field lines in gray solid lines. The white solid lines indicate the radial infall sonic transition at –0.2 km s<sup>–1</sup>. The thick black dashed line indicates the positions where the material is 90% Keplerian supported.<br> <b>Right:</b> the face-on view of the case with rotational axis and magnetic axis being anti-parallel. Note that the Hall effect forces the inner part to rotate in a direction opposite to that of the outer part.
Disk Formation Enabled by the Hall Effect
Snapshots of 2D density distributions of models with different mangetization, at a representative time of 10<sup>12</sup> sec. The white solid lines indicate positions of the radial infall sonic transition at –0.2 km s<sup>–1</sup>, and the dark gray solid lines mark the positions with 100% Keplerian rotational support. The top panels show two close-to-extreme cases: the non-magnetic case with no magnetic breaking <b>(left)</b> and the ideal-MHD case where no rotationally supported disks form <b>(right)</b>. The bottom panels show magnetic cases but with enhanced resistivity. The case with 10<sup>20</sup> cm<sup>2</sup> s<sup>–1</sup> forms a rotationally supported disk on a scale of ~ 100 AU.
Disk Formation Enabled by Enhanced Resistivity
In the bottom panels, square sections of surface density simulated with <b>Antares</b> are shown centered at the locations of protoplanets. The surface density is obtained by vertical integration over <i>z</i> < 0.0156 AU (the height of the finest level) for protoplanets with masses of 4, 8, and 16 Earth Masses, respectively. The central star is located on the left and the protoplanets are orbiting the central star counterclockwise. On top of each surface density is the corresponding volume density cutting through the plane defined by
Formation of Isothermal Circumplanetary Disks with Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets
<b>Left:</b> near infrared [Fe II] 1.644 µm + continuum image of the wide binary FS Tau A and B. FS Tau B is not visible but its adjacent reflection nebula R3 is bright in continuum. Jet and counterjet driven from FS Tau B along 55 degrees are indicated. <br> <b>Right:</b> continuum-subtracted position-velocity diagram of FS Tau B jet in [Fe II] along the position angle of the jet. The position of the invisible driving source is indicated by the horizontal dashed line and the systemic velocity is labeled by the vertical dash-dotted line. The blueshifted and redshifted knots have velocities -74.6 and +55.8 km/s, respectively.
Is FS Tau B Driving an Asymmetric Jet?
Figure (a) shows the normalized line profiles of the Ne II 12.81um (blue), Ne III 15.55um (red), and the O I 6300 (black) lines for a X-Wind jet modeled for a typical T Tauri star, at an inclination angle of 45 degrees. Figure (b) shows the contribution of the Ne II line as a function of cylindrical distance to the jet axis.
Neon Fine-Structure Line Emission from the Outflows of Young Stellar Objects
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學經歷

  • NanoSIMS Co-lead (2017~ 迄今)
  • CompAS Group Lead (2017~ 迄今)
  • Research Fellow (2022~ 迄今)
  • PI Charms Project (2008~ 迄今)
  • 長聘副研究員 (2013~2021)
  • 副研究員 (2007~2012)
  • Manager, Theoretical Institute for Advanced Research in Astrophysics (TIARA) (2005~2017)
  • Assistant Research Fellow, ASIAA (2000~2007)
  • Visiting Scientist, Harvard-Smithsonian Center for Astrophysics (2000~2003)
  • Postdoctral Fellow, Harvard-Smithsonian Center for Astrophysics (1999~2000)
  • Postdoctral Researcher, UC Berkeley (1998~1999)
  • Ph.D., Astronomy, UC Berkeley (1998)
  • PhD Advisor: Frank H. Shu (1998)
  • M.A, Biophysics, UC Berkeley (1994)
  • B.S, Physics, National Taiwan University (1991)

榮譽與獎勵

  • Outstanding Scholar Award (2002~2004)
  • Berkeley-Illinois-Maryland Association (BIMA) scholarship, ASIAA (1994~1998)
  • Outstanding Graduate Student Instructor Award, Physics, UC Berkeley (1994)

委員會服務

  • ALMA Proposal Review Panel, Cycle 6, Panel Chair in Category 3 (2018)
  • ALMA Proposal Review Panel, Cycle 5, Panel Chair in Category 3 (2017)
  • ALMA Proposal Review Panel, Cycle 4 (2016)
  • Biocomplex 2015: 2015 Taipei International Workshop for Soft Matter and Biophysics (2015)
  • 7th North American ALMA Science Workshop, Transformational Science with ALMA: From Dust to Rocks to Planets Formation and Evolution of Planetary Systems, Co-Chair (2013)
  • Lin-Shu Symposium: Fifty Years of Density Waves, Chair (2013)
  • Star Formation and the Interstellar Medium: Thirty-Five Years Later (2012)
  • 6th North American ALMA Science Workshop, Winds, Outflows, and Jets: from Young Stars to Supermassive Blackholes, Chair (2012)
  • Subcommittee of AS Computing Budget Review for Physical Sciences (2012)
  • Advisory Committee of Academia Sinica Information Security (2011~2013)
  • Extending the Limits of Astrophysical Spectroscopy (2011)
  • Advisory Committee for Academia Sinica Computing Center (2010~2014)
  • Fourth East Asian Numerical Astrophysics Meeting (EANAM) (2010)
  • Workshop on “From Chemistry to Life”, Western Pacific Geophysical Meeting, Convenor (2010)
  • IAU General Assembly 2009, Special Session 7: Young Stars, Brown Dwarfs, and Protoplanetary Disks (2009)
  • ALMA North American Science Advisory Committee (ANASAC) (2008~2012)
  • Center for Star Formation Studies (CSFS): Star Formation Workshop 2002, Chair (2002)

所屬專業及學術團體

  • International Astronomical Union (2010~ 迄今)
  • American Astronomical Society (1996~ 迄今)

研究興趣

Theoretical and Computational Astrophysics; Clouds, Collapse, Jets/Winds/Outflows; Protoplanetary and Circumplanetary Disks, Magnetic Field, Astrochemistry; Origins of Solar Systems, Meteorites, Planetary material, CAIs, Chondrules, and Isotopes; Numerical Methods, High-Performance Computing, GPU; Visualization

研究著作

查詢ADS上的研究著作

期刊論文(中研院就職期間發表)

  1. Ai T-H; Liu C-F; Shang H; Johnstone D; Krasnopolsky R, "A Unified Model for Bipolar Outflows from Young Stars: Kinematic and Mixing Structures in HH 30" , ApJ: 964(2), id.147 (15 pp), Apr, 2024 [SCI] ( ADS | Fulltext )
  2. Almenara JM; Bonfils X; Bryant EM; Jordán A; Hébrard G; Martioli E; Correia ACM; Astudillo-Defru N; Cadieux C; Arnold L; Artigau Ù; Bakos GÑ; Barros SCC; Bayliss D; Bouchy F; Boué G; Brahm R; Carmona A; Charbonneau D; Ciardi DR; Cloutier R; Cointepas M; Cook NJ; Cowan NB; Delfosse X; Dias Do Nascimento J; Donati JF; Doyon R; Forveille T; Fouqué P; Gaidos E; Gilbert EA; Gomes Da Silva J; Hartman JD; Hesse K; Hobson MJ; Jenkins JM; Kiefer F; Kostov VB; Laskar J; Lendl M; L'heureux A; Martins JHC; Menou K; Moutou C; Murgas F; Polanski AS; Rapetti D; Sedaghati E; Shang H, "TOI-4860 b, a short-period giant planet transiting an M3.5 dwarf" , A&A: 683, id.A166 (16pp), Mar, 2024 [SCI] ( ADS | Fulltext )
  3. Hirotani K; Shang H; Krasnopolsky R; Nishikawa K, "Formation of Limb-brightened Radio Jets by Angle-dependent Energy Extraction from Rapidly Rotating Black Holes" , ApJ: 965(1), id.50 (11 pp), Apr, 2024 [SCI] ( ADS | Fulltext )
  4. Motoyama K; Krasnopolsky R; Shang H; Aida K; Sakane E, "An Efficient Algorithm for Astrochemical Systems Using Stoichiometry Matrices" , ApJS: 270(2), id.19 (11 pp), Jan, 2024 [SCI] ( ADS | Fulltext )
  5. Allart R; Lemée-Joliecoeur PB; Jaziri AY; Lafrenière D; Artigau E; Cook N; Darveau-Bernier A; Dang L; Cadieux C; Boucher A; Bourrier V; Deibert EK; Pelletier S; Radica M; Benneke B; Carmona A; Cloutier R; Cowan NB; Delfosse X; Donati JF; Doyon R; Figueira P; Forveille T; Fouqué P; Gaidos E; Gu PG; Hébrard G; Kiefer F; Kóspál Ñ; Jayawardhana R; Martioli E; Dos Santos LA; Shang H; Turner JD; Vidotto AA, "Homogeneous search for helium in the atmosphere of 11 gas giant exoplanets with SPIRou" , A&A: 677, id.A164 (26 pp), Sep, 2023 [SCI] ( ADS | Fulltext )
  6. Feeney-Johansson A; Purser SJD; Ray TP; Carrasco-González C; Rodríguez-Kamenetzky A; Eislöffel J; Lim J; Galván-Madrid R; Lizano S; Rodríguez LF; Shang H; Ho P; Hoare M, "A high-resolution radio study of the L1551 IRS 5 and L1551 NE jets" , A&A: 677, id.A97 (13 pp), Sep, 2023 [SCI] ( ADS | Fulltext )
  7. Hirotani K; Shang H; Krasnopolsky R; Nishikawa K-I, "Two-dimensional Particle-in-Cell simulations of axisymmetric black hole magnetospheres: angular dependence of the Blandford-Znajek flux" , ApJ: 943(2), id.164 (19 pp.), Feb, 2023 [SCI] ( ADS | Fulltext )
  8. Hsu S-Y; Liu S-Y; Johnstone D; Liu T; Bronfman L; Chen H-RV; Dutta S; Eden DJ; Evans NJ, Ii; Hirano N; Juvela M; Kuan Y-J; Kwon W; Lee C-F; Lee CW; Lee J-E; Li S; Liu C-F; Liu X; Luo Q; Qin S-L; Rawlings MG; Sahu D; Sanhueza P; Shang H; Tatematsu K; Yang Y-L, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): The Warm-Envelope Origin of Hot Corinos" , ApJ: 956(2), id.120 (23pp), Oct, 2023 [SCI] ( ADS | Fulltext )
  9. Kiefer F; Hébrard G; Martioli E; Artigau E; Doyon R; Donati J-F; Cadieux C; Carmona A; Ciardi DR; Cristofari PI; de Almeida L; Figueira P; Gaidos E; Gonzales E; Lecavelier Des Etangs A; Stassun KG; Arnold L; Benneke B; Boisse I; Bonfils X; Cook NJ; Cortés-Zuleta P; Delfosse X; do Nascimento JD; Fausnaugh M; Fong W; Fouqué P; Forveille T; Gomes da Silva J; Hesse K; Kóspál Á; Lewis H; Liu C-F; Martins JHC; Paegert M; Seager S; Shang H; Twicken JD; Vandal T; Vinatier S; Widemann T; Winn JN, "A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS" , A&A: 670, id.A136 (28 pp), Feb, 2023 [SCI] ( ADS | Fulltext )
  10. Luo Q-Y; Liu T; Lee AT; Offner SSR; Di Francesco J; Johnstone D; Juvela M; Goldsmith PF; Qin S-L; Mai X; Liu X-C; Sanhueza P; Xu F-W; Tatematsu KI; Dutta S; Chen H-RV; Li S; Yang A; Liu S-Y; Lee C-F; Hirano N; Lee CW; Sahu D; Shang H; Hsu S-Y; Bronfman L; Kwon W; Rawlings MG; Eden D; Lu X; Gu Q-L; Ren Z; Ward-Thompson D; Shen Z-Q, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Forming Quadruple System with Continuum "Ribbons" and Intricate Outflows" , ApJL: 952(1), L2 (10 pp), July, 2023 [SCI] ( ADS | Fulltext )
  11. Sahu D; Liu S-Y; Johnstone D; Liu T; Evans NJ, Ii; Hirano N; Tatematsu KI; Di Francesco J; Lee C-F; Kim K-T; Dutta S; Hsu S-Y; Li S; Luo Q-Y; Sanhueza P; Shang H; Traficante A; Juvela M; Lee CW; Eden DJ; Goldsmith PF; Bronfman L; Kwon W; Lee J-E; Kuan Y-J; Ristorcelli I, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Density Structure of Centrally Concentrated Prestellar Cores from Multiscale Observations" , ApJ: 945 (2), id.156 (15pp), March, 2023 [SCI] ( ADS | Fulltext )
  12. Shang H; Krasnopolsky R; Liu C-F, "A Unified Model for Bipolar Outflows from Young Stars: Apparent Magnetic Jet Acceleration" , ApJL: 945(1), id.L1 (21 pp), March, 2023 [SCI] ( ADS | Fulltext )
  13. Shang H; Liu C-F; Krasnopolsky R; Wang L-Y, "A Unified Model for Bipolar Outflows from Young Stars: Kinematic Signatures of Jets, Winds, and Their Magnetic Interplay with the Ambient Toroids" , ApJ: 944(2), id.230 (55 pp), Feb, 2023 [SCI] ( ADS | Fulltext )
  14. Takami M; Guenther HM; Schneider PC; Beck TL; Karr JL; Ohyama Y; Galvan-Madrid R; Uyama T; White M; Grankin K; Coffey D; Liu C-F; Fukagawa M; Manset N; Chen W-P; Pyo T-S; Shang H; Ray TP; Otsuka M; Chou M-Y, "Time-variable Jet Ejections from RW Aur A, RY Tau, and DG Tau" , ApJS: 264(1), id.1 (19pp), Jan, 2023 [SCI] ( ADS | Fulltext )
  15. Väisälä MS; Shang H; Galli D; Lizano S; Krasnopolsky R, "Exploring the Formation of Resistive Pseudodisks with the GPU Code Astaroth" , ApJ: 959(1), id.32 (21pp), Dec, 2023 [SCI] ( ADS | Fulltext )
  16. Bandopadhyay S; Shang H, "SADHANA: A Doubly Linked List-based Multidimensional Adaptive Mesh Refinement Framework for Solving Hyperbolic Conservation Laws with Application to Astrophysical Hydrodynamics and Magnetohydrodynamics" , ApJS: 263(2), id.32 (25pp), Dec, 2022 [SCI] ( ADS | Fulltext )
  17. Cemeljic M; Yang H; Yuan F; Shang H, "Formation of episodic jets and associated flares from black hole accretion systems" , ApJ: 933(1), id.55 (13pp), July, 2022 [SCI] ( ADS | Fulltext )
  18. Dutta S; Lee C-F; Hirano N; Liu T; Johnstone D; Liu S-Y; Tatematsu K; Goldsmith PF; Sahu D; Evans NJ; Sanhueza P; Kwon W; Qin S-L; Ranjan Samal M; Zhang Q; Kim K-T; Shang H; Lee CW; Moraghan A; Jhan K-S; Li S; Lee J-E; Traficante A; Juvela M; Bronfman L; Eden D; Soam A; He J; Liu H-L; Kuan Y-J; Pelkonen V-M; Luo Q; Yi H-W; Hsu S-Y, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Evidence for a Molecular Jet Launched at an Unprecedented Early Phase of Protostellar evolution" , ApJ: 931(2), id.130 (13pp), June, 2022 [SCI] ( ADS | Fulltext )
  19. Dutta S; Lee C-F; Johnstone D; Liu T; Hirano N; Liu S-Y; Lee J-E; Shang H; Tatematsu KI; Kim K-T; Sahu D; Sanhueza P; Di Francesco J; Jhan K-S; Lee CW; Kwon W; Li S; Bronfman L; Liu H-L; Traficante A; Kuan Y-J; Hsu S-Y; Moraghan A; Liu C-F; Eden D; Soam A; Luo Q; ALMASOP Team, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of a Dense SiO Jet in the Evolved Protostellar Phase" , ApJ: 925(1), id.11 (10pp), Jan, 2022 [SCI] ( ADS | Fulltext )
  20. Hsu S-Y; Liu S-Y; Liu T; Sahu D; Lee C-F; Tatematsu K; Kim K-T; Hirano N; Yang Y-L; Johnstone D; Liu H; Juvela M; Bronfman L; Chen H-RV; Dutta S; Eden DJ; Jhan K-S; Kuan Y-J; Lee CW; Lee J-E; Li S; Liu C-F; Qin S-L; Sanhueza P; Shang H; Soam A; Traficante A; Zhou J, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Hot Corino Survey toward Protostellar Cores in the Orion Cloud" , ApJ: 927(2), id.218 (27pp), March, 2022 [SCI] ( ADS | Fulltext )
  21. Jhan K-S; Lee C-F; Johnstone D; Liu T; Liu S-Y; Hirano N; Tatematsu KI; Dutta S; Moraghan A; Shang H; Lee J-E; Li S; Liu C-F; Hsu S-Y; Kwon W; Sahu D; Liu X-C; Kim K-T; Luo Q; Qin S-L; Sanhueza P; Bronfman L; Qizhou Z; Eden D; Traficante A; Lee CW; Almasop T, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Deriving Inclination Angle and Velocity of the Protostellar Jets from Their SiO Knots" , ApJL: 931(1), id.L5 (9pp), May, 2022 [SCI] ( ADS | Fulltext )
  22. Johnstone D; Lalchand B; Mairs S; Shang H; Chen WP; Bower GC; Herczeg GJ; Lee J-E; Forbrich J; Chen B-Y; Contreras Peña C; Lee Y-H; Park W; Broughton C; Plovie S; Team JT, "The JCMT Transient Survey: Single-epoch Transients and Variability of Faint Sources" , ApJ: 937(1), id.6 (12pp), Sep, 2022 [SCI] ( ADS | Fulltext )
  23. Lee C-F; Li Z-Y; Shang H; Hirano N, "Magnetocentrifugal Origin for Protostellar Jets Validated through Detection of Radial Flow at the Jet Base" , ApJ: 927(2), id.L27 (8pp), March, 2022 [SCI] ( ADS | Fulltext )
  24. Liu X; Liu T; Shen Z; Qin S-L; Luo Q; Cheng Y; Gu Q; Zhang T; Zhu F; Liu S-Y; Lu X; Zhao R; Zhong W; Wu Y; Li J; Zhao Z; Wang J; Liu Q; Xia B; Li B; Fu L; Yan Z; Zhang C; Wang L; Ye Q; Tatematsu KI; Liu H; Shang H; Xu F; Lee C-F; Zhang C; Dutta S, "A Q-band line survey towards Orion KL using the Tianma radio telescope" , ApJS: 263(1), id.13 (21 pp), Nov, 2022 [SCI] ( ADS | Fulltext )
  25. Rodríguez-Kamenetzky AR; Carrasco-González C; Rodríguez LF; Ray TP; Sanna A; Moscadelli L; Hoare M; Galván-Madrid R; Shang H; Lizano S; Eislöffel J; Lim J; Torrelles JM; Ho P; Feeney-Johansson A, "Resolving the Collimation Zone of an Intermediate-mass Protostellar Jet" , ApJL: 931(2), id.L26 (10pp), June, 2022 [SCI] ( ADS | Fulltext )
  26. Sanghani MN; Lajaunie L; Marhas KK; Rickard WDA; Hsiao SS-Y; Peeters Z; Shang H; Lee D-C; Calvino JJ; Bizzarro M, "Microstructural and Chemical Investigations of Presolar Silicates from Diverse Stellar Environments" , ApJ: 925(2), id.110 (28pp), Feb, 2022 [SCI] ( ADS | Fulltext )
  27. Wang W; Väisälä MS; Shang H; Krasnopolsky R; Li Z-Y; Lam KH; Yuan F, "Magnetic Spirals in Accretion Flows Originated from Misaligned Magnetic Fields" , ApJ: 928(1), id.85 (23pp), March, 2022 [SCI] ( ADS | Fulltext )
  28. Hirotani K; Krasnopolsky R; Shang H; Nishikawa K-I; Watson M, "Two-dimensional Particle-in-Cell Simulations of Axisymmetric Black Hole Magnetospheres" , ApJ: 908(1), id.88 (19pp), Feb, 2021 [SCI] ( ADS | Fulltext )
  29. Krasnopolsky R; Ponce-Martinez MP; Shang H; Tseng Y-H; Yen CC, "Efficient Direct Method for Self-gravity in 3D, Accelerated by a Fast Fourier Transform" , ApJS: 252(2), id.14 (14pp), Feb, 2021 [SCI] ( ADS | Fulltext )
  30. Lajaunie L; Sanghani M; Rickard W; Hsiao SS-Y; Peeters Z; Shang H; Lee D-C; Calvino J; Marhas K; Bizzarro M, "Isotopic, Structural and Chemical Analyses of Pre-Solar Silicates from Asymptotic Giant Branch Stars and Type-II Supernova Explosions" , Microscopy and Microanalysis: 27(S1), 2782-2784, Aug, 2021 ( ADS | Fulltext )
  31. Lee Y-H; Johnstone D; Lee J-E; Herczeg G; Mairs S; Contreras-Peña C; Hatchell J; Naylor T; Bell GS; Bourke TL; Broughton C; Francis L; Gupta A; Harsono D; Liu S-Y; Park G; Plovie S; Moriarty-Schieven GH; Scholz A; Sharma T; Teixeira PS; Wang Y-T; Aikawa Y; Bower GC; Chen H-RV; Bae J; Baek G; Chapman S; Chen WP; Du F; Dutta S; Forbrich J; Guo Z; Inutsuka S-I; Kang M; Kirk H; Kuan Y-J; Kwon W; Lai S-P; Lalchand B; Lane JMM; Lee C-F; Liu T; Morata O; Pearson S; Pon A; Sahu D; Shang H; Stamatellos D; Tang S-Y; Xu Z; Yoo H; Rawlings JMC, "The JCMT Transient Survey: Four-year Summary of Monitoring the Submillimeter Variability of Protostars" , ApJ: 920(2), id.119 (23pp), Oct, 2021 [SCI] ( ADS | Fulltext )
  32. Liu C-F; Shang H; Herczeg GJ; Walter FM, "Revealing Ionization Conditions of Sz 102 with Spatially Resolved [Ne III] Microjets" , ApJ: 909(2), id.196 (12pp), Mar, 2021 [SCI] ( ADS | Fulltext )
  33. Mannfors E; Juvela M; Bronfman L; Eden DJ; He J; Kim G; Kim K-T; Kirppu H; Liu T; Montillaud J; Parsons H; Sanhueza P; Shang H; Soam A; Tatematsu K; Traficante A; Väisälä MS; Lee CW, "Characterization of dense Planck clumps observed with Herschel and SCUBA-2" , A&A: 654, id.A123 (54pp), Oct, 2021 [SCI] ( ADS | Fulltext )
  34. Sahu D; Liu S-Y; Liu T; Evans NJ, Ii; Hirano N; Tatematsu KI; Lee C-F; Kim K-T; Dutta S; Alina D; Bronfman L; Cunningham M; Eden DJ; Garay G; Goldsmith PF; He J; Hsu S-Y; Jhan K-S; Johnstone D; Juvela M; Kim G; Kuan Y-J; Kwon W; Lee CW; Lee J-E; Li D; Li PS; Li S; Luo Q-Y; Montillaud J; Moraghan A; Pelkonen V-M; Qin S-L; Ristorcelli I; Sanhueza P; Shang H; Shen Z-Q; Soam A; Wu Y; Zhang Q; Zhou J, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of Extremely High-density Compact Structure of Prestellar Cores and Multiple Substructures Within" , ApJL: 907(1), L15 (9pp), Jan, 2021 [SCI] ( ADS | Fulltext )
  35. Sanghani M; Marhas K; Hsiao SS-Y; Peeters Z; Shang H; Lee D-C; Bizzarro M, "Presolar Silicate and Oxide Grains Found in Lithic Clasts from Isheyevo and the Fine-grained Matrix of Northwest Africa 801" , ApJS: 253(2), id.41 (26pp), Apr, 2021 [SCI] ( ADS | Fulltext )
  36. Väisälä MS; Pekkilä J; Käpylä MJ; Rheinhardt M; Shang H; Krasnopolsky R, "Interaction of Large- and Small-scale Dynamos in Isotropic Turbulent Flows from GPU-accelerated Simulations" , ApJ: 907(2), id.83 (18pp.), Feb, 2021 [SCI] ( ADS | Fulltext )
  37. Zhao B; Caselli P; Li Z-Y; Krasnopolsky R; Shang H; Lam KH, "The Interplay between Ambipolar Diffusion and Hall Effect on Magnetic Field Decoupling and Protostellar Disc Formation" , MNRAS: 505(4), 5142-5163, Aug, 2021 [SCI] ( ADS | Fulltext )
  38. Dutta S; Lee CF; Liu T; Hirano N; Liu SY; ... ; Shang H; Sahu D;...; Moraghan A; Jhan KS; Hsu SY;...; Kuan YJ; et al., "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP). II. Survey Overview: A First Look at 1.3 mm Continuum Maps and Molecular Outflows" , ApJS: 251(2), id.20 (35pp.), Dec, 2020 [SCI] ( ADS | Fulltext )
  39. Hsu SY; Liu SY; ...; Sahu D; Hirano N; Lee CF; ...; Dutta S; ...; Jhan K-S; ...; Kuan YJ; ...; Moraghan A; ...; Shang H, "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP). I. Detection of New Hot Corinos with the ACA" , ApJ: 898(2), id.107 (37pp.), Aug, 2020 [SCI] ( ADS | Fulltext )
  40. Shang H; Krasnopolsky R; Liu C-F; Wang L-Y, "A Unified Model for Bipolar Outflows from Young Stars: The Interplay of Magnetized Wide-angle Winds and Isothermal Toroids" , ApJ: 905(2), id.116 (52pp.), Dec, 2020 [SCI] ( ADS | Fulltext )
  41. Takami M; ...; Karr JL; Ohyama Y; ...; Liu HB; ...; Liu CF; ...; Shang H; ...; Chou MY, "Possible Time Correlation between Jet Ejection and Mass Accretion for RW Aur A" , ApJ: 901(1), id.24 (9pp.), Sep, 2020 [SCI] ( ADS | Fulltext )
  42. Yen H-W; Zhao B; Koch P; Krasnopolsky R; Li Z-Y; Ohashi N; Shang H; Takakuwa S; Tang Y-W, "Transition from Ordered Pinched to Warped Magnetic Field on a 100 au Scale in the Class 0 Protostar B335" , ApJ: 893(1), id.54 (11pp.), Apr, 2020 [SCI] ( ADS | Fulltext )
  43. Zhao B; Caselli P; Li Z-Y; Krasnopolsky R; Shang H; et al., "Hall effect in protostellar disc formation and evolution" , MNRAS: 492(3), 3375-3395, Mar, 2020 [SCI] ( ADS | Fulltext )
  44. Eden DJ; Liu T; Kim K-T; ...; Liu S-Y; ...; Hirano N; ...; Koch PM; ...; Chu YH; ...; Lai SP; Lee CF; ...; Morata O; ...; Pech G; ...; Shang H; ...; Tang YW; et al., "SCOPE: SCUBA-2 Continuum Observations of Pre-protostellar Evolution - survey description and compact source catalogue" , MNRAS: 485(2), 2895-2908, May, 2019 [SCI] ( ADS | Fulltext )
  45. Suriano SS; Li Z-Y; Krasnopolsky R; ...; Shang H; et al., "The formation of rings and gaps in wind-launching non-ideal MHD discs: three-dimensional simulations" , MNRAS: 484(1), 107-124, Mar, 2019 [SCI] ( ADS | Fulltext )
  46. Tseng Y-H; Shang H; Yen C-C, "Direct Calculation of Self-gravitational Force for Infinitesimally Thin Gaseous Disks Using Adaptive Mesh Refinement" , ApJS: 244(2), id. 26 (13 pp.), Oct, 2019 [SCI] ( ADS | Fulltext )
  47. Vaisala M; Shang H; Krasnopolsky R; Liu S-Y; et al., "Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes" , ApJ: 873(2), id. 114 (22 pp.), Mar, 2019 [SCI] ( ADS | Fulltext )
  48. Wang L-Y; Shang H; Chiang T-Y, "Ejection History of the IRAS 04166+2706 Molecular Jet" , ApJ: 874(1), id. 31 (12 pp.), Mar, 2019 [SCI] ( ADS | Fulltext )
  49. Lee C-F; Li Z-Y; Hirano N; Shang H; Ho PTP; et al., "ALMA Observations of the Very Young Class 0 Protostellar System HH211-mms: A 30 au Dusty Disk with a Disk Wind Traced by SO?" , ApJ: 863(1), id. 94 (9 pp.), Aug, 2018 [SCI] ( ADS | Fulltext )
  50. Lee CF; Li ZY; Codella C; Ho PTP; Podio L; Hirano N; Shang H; et al., "A 100 au Wide Bipolar Rotating Shell Emanating from the HH 212 Protostellar Disk: A Disk Wind?" , ApJ: 856(1), id. 14 (13 pp.), March 20, 2018 [SCI] ( ADS | Fulltext )
  51. Liu T; Kim K-T; Juvela M; ...; Liu S-Y; ...; Koch PM; ...; Hirano N; ...; Chen H-R; Lee C-F; ...; Morata O; ...; Shang H; ...; Tang Y-W; et al., "The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17" , ApJS: 234(2), 28, Feb, 2018 [SCI] ( ADS | Fulltext )
  52. Suriano SS; Li Z-Y; Krasnopolsky R; Shang H, "The formation of rings and gaps in magnetically coupled disk-wind systems: ambipolar diffusion and reconnection" , MNRAS: 477(1), 1239-1257, June, 2018 [SCI] ( ADS | Fulltext )
  53. van Kooten EMME; Cavalcante LL; Nagashima K; ...; Peeters Z; Hsiao SSY; Shang H; Lee DC; Lee T; et al., "Isotope record of mineralogical changes in a spectrum of aqueously altered CM chondrites" , GCA: 237, 79-102, Sep, 2018 [SCI] ( ADS | Fulltext )
  54. Lee C-F; Ho PTP; Li Z-Y; Hirano N; Zhang Q; Shang H, "A Rotating Protostellar Jet Launched from the Innermost Disk of HH 212" , Nature Astronomy: 1, 0152, July, 2017 [SCI] ( ADS | Fulltext )
  55. Lee C-F; Li Z-Y; Ho PTP; Hirano N; Zhang Q; Shang H, "First detection of equatorial dark dust lane in a protostellar disk at submillimeter wavelength" , Science Advances: 3(4), e1602935, April, 2017 [SCI] ( ADS | Fulltext )
  56. Lee C-F; Li Z-Y; Ho PTP; Hirano N; Zhang Q; Shang H, "Formation and Atmosphere of Complex Organic Molecules of the HH 212 Protostellar Disk" , ApJ: 843(1), 27, July 1, 2017 [SCI] ( ADS | Fulltext )
  57. Suriano SS; Li ZY; Krasnopolsky R; Shang H, "Rings and gaps produced by variable magnetic disc winds and avalanche accretion streams - I. Axisymmetric resistive MHD simulations" , MNRAS: 468(4), 3850-3868, July, 2017 [SCI] ( ADS | Fulltext )
  58. Tafalla M; Su Y-N; Shang H; ...; Lee C-F; Hirano N; Wang L-Y, "Anatomy of the internal bow shocks in the IRAS 04166+2706 protostellar jet" , A&A: 597, A119, Jan, 2017 [SCI] ( ADS | Fulltext )
  59. Liu C-F; Shang H; Herczeg GJ; Walter FM, "The [Ne III] Jet of DG Tau and Its Ionization Scenarios" , ApJ: 832(2), 153, Dec, 2016 [SCI] ( ADS | Fulltext )
  60. Zhao B; Caselli P; Li Z-Y; Krasnopolsky R; Shang H; Nakamura F, "Protostellar disc formation enabled by removal of small dust grains" , MNRAS: 460(2), 2050-2076, Aug 1, 2016 [SCI] ( ADS | Fulltext )
  61. Lee C-F; Hirano N; Zhang Q; Shang H; Ho PTP; et al., "Jet Motion, Internal Working Surfaces, and Nested Shells in the Protostellar System HH 212" , ApJ: 805(2), 186, June 1, 2015 [SCI] ( ADS | Fulltext )
  62. Motoyama K; Morata O; Shang H; Krasnopolsky R; Hasegawa T, "A hydrochemical hybrid code for astrophysical problems. I. Code verification and benchmarks for Photon-Dominated Region (PDR)" , ApJ: 808(1), 46, July, 2015 [SCI] ( ADS | Fulltext )
  63. Wang L-Y; Shang H; Krasnopolsky R; Chiang T-Y, "A Two-Temperature Model of Magnetized Protostellar Outflows" , ApJ: 815(1), 39, Oct 10, 2015 [SCI] ( ADS | Fulltext )
  64. Lee CF; Hirano N; Zhang QZ; Shang H; Ho PTP; Krasnopolsky R, "ALMA Results of the Pseudodisk, Rotating Disk, and Jet in the Continuum and HCO+ in the Protostellar System HH 212" , ApJ: 786(2), 114, May, 2014 [SCI] ( ADS | Fulltext )
  65. Li Z-Y; Banerjee R; Pudritz RE; Jørgensen JK; Shang H; Krasnopolsky R; Maury A, "The Earliest Stages of Star and Planet Formation: Core Collapse, and the Formation of Disks and Outflows" , Protostars and Planets: VI, 173-194, 2014 ( ADS | Fulltext )
  66. Li ZY; Krasnopolsky R; Shang H; Zhao B, "On the Role of Pseudodisk Warping and Reconnection in Protostellar Disk Formation in Turbulent Magnetized Cores" , ApJ: 793(2), 130, Oct, 2014 [SCI] ( ADS | Fulltext )
  67. Liu C-F; Shang H; Walter FM; Herczeg GJ, "Velocity-resolved [Ne III] from X-Ray Irradiated Sz 102 Microjets" , ApJ: 786(2), 99, May, 2014 [SCI] ( ADS | Fulltext )
  68. Wang H-H; Bu D; Shang H; Gu P-G, "Formation of Isothermal Disks around Protoplanets. I. Introductory Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets" , ApJ: 790(1), 32, July, 2014 [SCI] ( ADS | Fulltext )
  69. Wang L-Y; Shang H; Su Y-N; ...; Hirano N; Lee C-F; et al., "Molecular Jet of IRAS 04166+2706" , ApJ: 780(1), 49, Jan, 2014 [SCI] ( ADS | Fulltext )
  70. Bu D; Shang H; Yuan F, "The effects of viscosity on circumplanetary disks" , RAA: 13(1), 71-86, Jan, 2013 [SCI] ( ADS | Fulltext )
  71. Cemeljic M; Shang H; Chiang TY, "Magnetospheric accretion and ejection of matter in resistive magnetohydrodynamic simulations" , ApJ: 768(1), 5, May 1, 2013 [SCI] ( ADS | Fulltext )
  72. Chou M-Y; Takami M; ...; Karr JL; Shang H; Liu HB, "Time Variability of Emission Lines for Four Active T Tauri Stars. I. October-December in 2010" , AJ: 145(4), 108, April, 2013 [SCI] ( ADS | Fulltext )
  73. Li Z-Y; Krasnopolsky R; Shang H, "Does Magnetic-field-Rotation Misalignment Solve the Magnetic Braking Catastrophe in Protostellar Disk Formation?" , ApJ: 774(1), 82, Sept 1, 2013 [SCI] ( ADS | Fulltext )
  74. Molnar S; Broadhurst T; Umetsu K; et al., "Tangential Velocity of the Dark Matter in the Bullet Cluster from Precise Lensed Image Redshifts" , ApJ: 774(1), 70, Sept 1, 2013 [SCI] ( ADS | Fulltext )
  75. Motoyama K; Umemoto T; Shang H; Hasegawa T, "Effects of Magnetic Field and Far-ultraviolet Radiation on the Structures of Bright-rimmed Clouds" , ApJ: 766(1), 50, Mar 20, 2013 [SCI] ( ADS | Fulltext )
  76. Krasnopolsky R; Li Z-Y; Shang H; Zhao B, "Protostellar Accretion Flows Destabilized by Magnetic Flux Redistribution" , ApJ: 757(1), 77, Sept 20, 2012 [SCI] ( ADS | Fulltext )
  77. Liu C-F; Shang H, "RW Aur A from the X-Wind Point of View: General Features" , ApJ: 761(2), 94, Dec, 2012 [SCI] ( ADS | Fulltext )
  78. Liu C-F; Shang H; Pyo T-S; Takami M; ...; Yan C-H; Wang SY; Ohashi N; Hayashi M, "Is FS Tau B Driving an Asymmetric Jet?" , ApJ: 749(1), 62, April 10, 2012 [SCI] ( ADS | Fulltext )
  79. Krasnopolsky R; Li Z-Y; Shang H, "Disk Formation in Magnetized Clouds Enabled by the Hall Effect" , ApJ: 733(1), 54, May 20, 2011 [SCI] ( ADS | Fulltext )
  80. Li Z-Y; Krasnopolsky R; Shang H, "Non-ideal MHD Effects and Magnetic Braking Catastrophe in Protostellar Disk Formation" , ApJ: 738(2), 180, Sept 10, 2011 [SCI] ( ADS | Fulltext )
  81. Zhao B; Li Z-Y; Nakamura F; Krasnopolsky R; Shang H, "Magnetic Flux Expulsion in Star Formation" , ApJ: 742(1), 10, Nov 20, 2011 [SCI] ( ADS | Fulltext )
  82. Hirano N; Ho PTP; Liu SY; Shang H; Lee CF;et al., "Extreme active molecular jets in L1448C" , ApJ: 717(1), 58-73, July 1, 2010 [SCI] ( ADS | Fulltext )
  83. Krasnopolsky R; Li Z-Y; Shang H, "Disk Formation Enabled by Enhanced Resistivity" , ApJ: 716(2), 1541-1550, June 20, 2010 [SCI] ( ADS | Fulltext )
  84. Lee CF; Hasegawa TI; Hirano N; Palau A; Shang H; Ho PTP; Zhang Q, "The Reflection-Symmetric Wiggle of the Young Protostellar Jet HH211" , ApJ: 713(2), 731-737, April 20, 2010 [SCI] ( ADS | Fulltext )
  85. Shang H; Glassgold AE; Lin W-C; Liu C-F, "Ne II Fine-structure Line Emission from the Outflows of Young Stellar Objects" , ApJ: 714(2), 1733-1739, May, 2010 [SCI] ( ADS | Fulltext )
  86. Krasnopolsky R; Shang H; Li Z-Y, "Topologies of Current-Free Axisymmetric Magnetospheres in Star-Disk Systems" , ApJ: 703(2), 1863-1871, Oct 1, 2009 [SCI] ( ADS | Fulltext )
  87. Lee CF; Hirano N; ...; Ho PTP; ...; Shang H, "Rotation and Outflow motions in the very low-mass Class 0 protostellar system HH 211 at subarcsecond resolution" , ApJ: 699(2), 1584-1594, July, 2009 [SCI] ( ADS | Fulltext )
  88. Cai MJ; Shang H; Lin HH; Shu FH, "X-winds in action" , ApJ: 672(1), 489-503, Jan 1, 2008 [SCI] ( ADS | Fulltext )
  89. Lee CF; Ho PTP; ...; Hirano N; Shang H; et al., "SiO shocks of the protostellar jet HH 212: A search for jet rotation" , ApJ: 685(2), 1026-1032, Oct 1, 2008 [SCI] ( ADS | Fulltext )
  90. Phan-Bao N; ...; Lee CF; Tang YW; Ho PTP; ...; Lim J; Ohashi N; Shang H, "First Confirmed Detection of a Bipolar Molecular Outflow from a Young Brown Dwarf" , ApJ: 689(2), L141-L144, Dec 20, 2008 [SCI] ( ADS | Fulltext )
  91. Lee CF; Ho PTP; Beuther H; Bourke TL; Hirano N; Shang H; Zhang Q, "HH212: SMA Observations of a Remarkable Protostellar Jet" , ApJ: 659(1), 499-511, Apr 10, 2007 [SCI] ( ADS | Fulltext )
  92. Lee CF; Ho PTP; Palau A; Hirano N; Bourke TL; Shang H; Zhang Q, "Submillimeter Arcsecond-Resolution Mapping of the Highly Collimated Protostellar Jet HH211" , ApJ: 670(2), 1188-1197, Dec 1, 2007 [SCI] ( ADS | Fulltext )
  93. Motoyama K; Umemoto T; Shang H, "A Radiation Driven Implosion Model for the Enhanced Luminosity of Protostars near HII Regions" , A&A: 467(2), 657-664, May, 2007 [SCI] ( ADS | Fulltext )
  94. Shang H, "Jets and molecular outflows from Herbig-Haro objects" , Ap&SS: 311(1-3), 25-34, Oct, 2007 [SCI] ( ADS | Fulltext )
  95. Shang H; Li Z-Y; Hirano N, "Jets and Bipolar Outflows from Young Stars: Theory and Observational Tests" , Protostars and Planets: V, 261-276, 2007 ( ADS | Fulltext )
  96. Gounelle M; Shu F; Shang H; Glassgold AE; Rehm KE; Lee T, "The Irradiation Origin of Beryllium Radioisotopes and Other Short-lived Radionuclides" , ApJ: 640(2), 1163-1170, Apr 1, 2006 [SCI] ( ADS | Fulltext )
  97. Hirano N; Liu SY; Shang H; Ho PTP; ...; Kuan YJ; et al., "SiO J=5-4 in the HH 211 protostellar jet imaged with the Submillimeter Array" , ApJ: 636(2), L141-L144, Jan 10, 2006 [SCI] ( ADS | Fulltext )
  98. Lee CF; Ho PTP; Beuther H; ...; Hirano N; Shang H, "Infall and Outflow around the HH 212 Protostellar System" , ApJ: 639 (1), 292-302, Mar 1, 2006 [SCI] ( ADS | Fulltext )
  99. Palau A; Ho PTP; Zhang Q; ...; Hirano N; Shang H;...; Kuan YJ, "Submillimeter emission from the hot molecular jet HH 211" , ApJ: 636(2), L137-L140, Jan 10, 2006 [SCI] ( ADS | Fulltext )
  100. Shang H; Allen A; Li Z-Y; Liu C-F; Chou M-Y; Anderson J, "A Unified Model for Bipolar Outflows from Young Stars" , ApJ: 649(2), 845-855, Oct, 2006 [SCI] ( ADS | Fulltext )
  101. Favata F; Flaccomio E; ...; Shang H; et al., "Bright X-Ray Flares in Orion Young Stars from COUP: Evidence for Star-Disk Magnetic Fields?" , ApJS: 160(2), 469-502, Oct, 2005 [SCI] ( ADS | Fulltext )
  102. Tsujimoto M; Feigelson ED; Grosso N; ...; Shang H; et al., "Iron Fluorescent Line Emission from Young Stellar Objects in the Orion Nebula" , ApJS: 160(2), 503-510, Oct, 2005 [SCI] ( ADS | Fulltext )
  103. Wolk SJ; Harnden FR; Flaccomio E; ...; Shang H; et al., "Stellar Activity on the Young Suns of Orion: COUP Observations of K5-7 PreMain-Sequence Stars" , ApJS: 160(2), 423-449, Oct, 2005 [SCI] ( ADS | Fulltext )
  104. Shang H, "Modeling Outflows from Young Stars" , IAUS: 221, 351-358, 2004 [SCI] ( ADS | Fulltext )
  105. Shang H; Lizano S; Glassgold A; Shu F, "Free-free Radio Emission from Young Stellar Objects" , ApJ: 612(1), L69-L72, Sept 1, 2004 [SCI] ( ADS | Fulltext )
  106. Shang H, "Developing Diagnostic Tools for X-Wind Jets" , Ap&SS: 287(1), 123-127, 2003 [SCI] ( ADS | Fulltext )
  107. Shang H; Glassgold AE; Shu FH; Lizano S, "Heating and ionization of X-winds" , ApJ: 564(2), 853-876, Jan, 2002 [SCI] ( ADS | Fulltext )
  108. Gounelle M; Shu FH; Shang H; ...; Lee T, "Extinct radioactivities and protosolar cosmic rays: Self-shielding and light elements" , ApJ: 548(2), 1051-1070, Feb 20, 2001 [SCI] ( ADS | Fulltext )
  109. Shang, Hsien, "Structure and Physical Conditions in MHD Jets from Young Stars" , JKAS: 34(4), 297-299, Dec, 2001 [SCI] ( ADS | Fulltext )
  110. Shu FH; Shang H; Gounelle M; Glassgold AE; Lee T, "The origin of chondrules and refractory inclusions in chondritic meteorites" , ApJ: 548(2), 1029-1050, Feb 20, 2001 [SCI] ( ADS | Fulltext )
  111. Shu FH; Shang H; Gounelle M; Glassgold AE; Lee T, "Making calcium-aluminum-rich inclusions and chondrules near the young sun by flares" , Meteorit Planet Sci: 35 Supplement, A145-A146, Sep, 2000 [SCI] ( ADS | Fulltext )
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