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Research Gallery

The Theoretical Institute for Advanced Research in Astrophysics (TIARA)

Neon Fine-Structure Line Emission from the Outflows of Young Stellar Objects Neon Fine-Structure Line Emission from the Outflows of Young Stellar Objects
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 ...(more)
“The First Hundred Million Years of the Solar System” workshop in November 2013 “The First Hundred Million Years of the Solar System” workshop in November 2013
“The First Hundred Million Years of the Solar System” workshop in November 2013 ...(more)
TIARA Winter School on Cosmology in February 2014 TIARA Winter School on Cosmology in February 2014
TIARA Winter School on Cosmology in February 2014 ...(more)
Numerical model for the asymmetric distribution of gas and dust column density maps of a face-on protoplanetary disk. Numerical model for the asymmetric distribution of gas and dust column density maps of a face-on protoplanetary disk.
Numerical model for the asymmetric distribution of gas (left panel) and dust (right panel) column density maps of a face-on protoplanetary disk. A massive giant planet (0.5% of the mass ...(more)
Stellar density wave of the spiral galaxy M81. Stellar density wave of the spiral galaxy M81.
Stellar density wave of the spiral galaxy M81. Left panel – Theoretical density distribution for a spiral mode. Middle panel – IRAC 3.6 micron map of the non-axisymmetric density distribution. ...(more)
TIARA 2013 Summer School on Astrobiology TIARA 2013 Summer School on Astrobiology
TIARA 2013 Summer School on Astrobiology ...(more)
TIARA 2012 Winter School on High Redshift Galaxies at ASIAA_2 TIARA 2012 Winter School on High Redshift Galaxies at ASIAA_2
TIARA 2012 Winter School on High Redshift Galaxies at ASIAA ...(more)
TIARA 2012 Winter School on High Redshift Galaxies at ASIAA TIARA 2012 Winter School on High Redshift Galaxies at ASIAA
TIARA 2012 Winter School on High Redshift Galaxies at ASIAA ...(more)
Star Formation Summer School at ASIAA in 2011 June_2 Star Formation Summer School at ASIAA in 2011 June_2
Star Formation Summer School at ASIAA in 2011 June ...(more)
Star Formation Summer School at ASIAA in 2011 June Star Formation Summer School at ASIAA in 2011 June
Star Formation Summer School at ASIAA in 2011 June ...(more)
TIARA Workshop TIARA Workshop "Star Formation through Spectroimaging at High Angular Resolution" held at ASIAA in 2011 June
TIARA Workshop "Star Formation through Spectroimaging at High Angular Resolution" held at ASIAA in 2011 June ...(more)
TIARA Workshop TIARA Workshop "Star Formation through Spectroimaging at High Angular Resolution" held at ASIAA in 2011 June.
TIARA Workshop "Star Formation through Spectroimaging at High Angular Resolution" held at ASIAA in 2011 June. ...(more)
Binary nature revealed in a spiral pattern of AFGL 3068 Binary nature revealed in a spiral pattern of AFGL 3068
A model comparison with an observed pinwheel spiral pattern of AFGL 3068: (a) The original Hubble Space Telescope image (Mauron & Huggins 2006), (b) the observed image overlaid with a ...(more)
Magnetospheric Accretion and Ejection of Matter in Resistive Magnetohydrodynamic Simulations Magnetospheric Accretion and Ejection of Matter in Resistive Magnetohydrodynamic Simulations
A schematic sketch of the evolution in star-disk interaction. ...(more)
AMR Study of the Common Envelope Phase of Binary Evolution AMR Study of the Common Envelope Phase of Binary Evolution
Gas density in the orbital plane of a binary system in the common envelope evolutionary phase. Gas quantities are sampled along the black line (see ApJ 746, 74), revealing the ...(more)
Non-thermal Emissions from Pulsars Non-thermal Emissions from Pulsars
The figure compares between the light curves (>100MeV) of the observation and the theory. ...(more)
The Existence of Inner Cool Disks in the Low Hard State of Accreting Black Holes The Existence of Inner Cool Disks in the Low Hard State of Accreting Black Holes
Schematic picture of the truncated outer disk separated from the inner disk by a coronal gap, indicating the energy and mass flow in the configuration. ...(more)
Death Line of Gamma-ray Pulsars with Outer Gaps Death Line of Gamma-ray Pulsars with Outer Gaps
Outer-gap death line on the period vs. derivative period plane. Left: entire parameter space. Right: close-up of the millisecond parameter range. ...(more)
Pulsed Gamma-Ray Emission from the Crab Pulsar Pulsed Gamma-Ray Emission from the Crab Pulsar
Phase-averaged spectrum of the pulsed emission from the Crab pulsar predicted by the self-consistent outer gap model. ...(more)
Spectral Hardening in the Trailing Peak of Gamma-ray Pulsar Light Curve Spectral Hardening in the Trailing Peak of Gamma-ray Pulsar Light Curve
Evolution of the photon index Γ (top panel) and the cutoff energy Ec (bottom panel) with the rotational phase is depicted by the (red) thick solid curve. ...(more)
On the Spiral Structure of NGC 5248: An Analytic Approach On the Spiral Structure of NGC 5248: An Analytic Approach
Comparisons between the observational intensity maps and the model images calculated from our theory for the galaxy NGC 5248. The left panels, from top to bottom, are B-band, CO (1-0), ...(more)
Evolution and Instability of a Self-gravitating Galactic Gaseous Disk under the Influence of a Fast Rotating Bar Potential Evolution and Instability of a Self-gravitating Galactic Gaseous Disk under the Influence of a Fast Rotating Bar Potential
Surface density for single OLR. Spiral waves are excited at 2kpc by a fast bar potential, lying in the horizontal direction. The high density spiral regions would lead to starbust ...(more)
X-ray and Gamma-ray Emissions from Rotation Powered Millisecond Pulsars X-ray and Gamma-ray Emissions from Rotation Powered Millisecond Pulsars
The results suggest that neutron stars in systems characterized by low thermal X-ray luminosities (i.e., SAX J1808-3658 and 1H 1905+000) may be of high mass. ...(more)
Theoretical Spectra of the AM CVn Binary System SDSS J0926+3624: Effects of Irradiation onto the Donor Star Theoretical Spectra of the AM CVn Binary System SDSS J0926+3624: Effects of Irradiation onto the Donor Star
It can be seen that the donor can reveal emission lines in the infrared region. Observations of both the continuum and lines in this wavelength region will provide important insight ...(more)
The Incidence of Non-spherical Circumstellar Envelopes in AGB Stars The Incidence of Non-spherical Circumstellar Envelopes in AGB Stars
The figures show the number of systems (color coded) for a degree of asymmetry, as measured by K, as a function of the orbital separation, luminosity, mass of the AGB ...(more)
Gravitationally Induced Density Wake of a Circularly Orbiting Object As an Interpretative Framework of Ubiquitous Spirals and Arcs Gravitationally Induced Density Wake of a Circularly Orbiting Object As an Interpretative Framework of Ubiquitous Spirals and Arcs
The above figures show the density enhancement of the spiral-onion shell shape (a) in the equatorial plane, (b) in a meridional plane, and (c) as a function of the distance ...(more)
On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars
A schematic view of binary system during the transition from the accretion powered low mass X-ray binary phase to the rotation powered millisecond radio pulsar phase. ...(more)
Triggered Formation of Young Stars Triggered Formation of Young Stars
Figure 1 shows DSS image of bright-rimmed cloud SFO21 whose ionizing star is located at 7 pc from the cloud. The arrow and diamond shows the direction of ionizing star ...(more)
Unified Model for Jets and Outflows from Young Stars Unified Model for Jets and Outflows from Young Stars
The figure shows the density structures at 100 (top) and 1000 (bottom) years with four representative numbers n = 1, 2, 4, 6 (from left to right), which indicates the ...(more)
Magnetization-Shaped Initial Mass Function Magnetization-Shaped Initial Mass Function
Schematic Initial Mass Function (Shu, Li, & Allen, 2004, ApJ, 601, 930) ...(more)
The Telescope of theory: synthetic SiO(7-6) emission from a young low-mass protostellar object embedded in an infall envelope The Telescope of theory: synthetic SiO(7-6) emission from a young low-mass protostellar object embedded in an infall envelope
SiO(7-6) image generated by non-LTE radiative transfer simulations along with MHD simulation. The low-mass (0.6 solar mass) object at the earliest stage of star formation shows significant irregular morphology compared ...(more)
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