| 1. Spiral Structure of
the Milky Way
With Professor C.C. Lin, I have established the overall spiral
structure of the Milky Way in late 60's and early 70's for the first
time. This spiral structure was achieved by comparing the density
wave theory and various observations: from optical to radio, from
stars to gas, from astrometry to kinematics. It has had significant
impact on the modern astronomy: (1) The consistency between the
theory and observations, on a wide range of observing aspects, has
constituted a convincing evidence for the validity of the theory.
(2) The spiral structure and the pattern speed of spiral waves determined
then are still widely used in the astronomy community until today.
Representative papers:
(1). C.C. Lin, Yuan, C., and F.H. Shu, "On
the Spiral Structure of Disk i Galaxies III. Comparison with Observations",
Ap.J. 155, 721 (1969). (SCI)
(2). Yuan, C.,"Application of
Density-Wave Theory to the Spiral Structure of the Milky Way System
I. Systematic Motion of Neutral Hydrogen", Ap.J., 158,
871 (1969). (SCI)
(3). Yuan, C.,"Application of Density Wave Theory to
the Spiral Structure of the Milky Way System II. Migration of Stars",
Ap. J. 158, 889 (1969). (SCI)
(4). C.C. Lin, Yuan, C., and W.W. Roberts, "On
the Stellar Streaming Motions and the Observational Determination
of
Structural Constant of the Galaxy", Astron. Astrophys.
69, 181-198 (1978). (SCI)
2. Galactic Magnetic Field
I used the fact that magnetic field and momentum flux of the gas
are both the divergent free in the frame rotating with the pattern
speed of the spiral density waves and thus made them proportional
to each other, i.e., B ~ u,
and solved the doubly periodic shock problem with the magnetized
interstellar medium (ISM) with Dr. Bill Roberts and showed the magnetic
shock coincides with the shock of ISM as well as the dust lanes
in 1970. The next year, Mathewson, van der Kruit and Brouw (1972)
discovered the enhancement of the synchrotron radiation along the
dust lane of M51, confirming the density wave theory. This galactic
model is still one of the best models describing the
overall configuration of galactic magnetic field in the galactic
plane.
(5) W.W. Roberts, Yuan, C., "Application
of Density-Wave Theory to the Spiral Structure of the Milky Way
System III. Galactic Magnetic Field", Ap.J. 161, 887
(1970). (SCI)
3. The "3-kpc Arm" Phenomenon
In 1983, I proposed that a fast rotating bar in the center of the
Milky Way is responsible for the "3-kpc Arm" phenomenon,
which had puzzled astronomer for a quarter of a century since its
discovery in late 50's. Both the linear and non-linear theory were
carried out to show that a small bar field can resonantly excite
spiral density waves with a non-linear radial outward streaming
motions of 53 km/s, as seen in the observations. The
existence of the central bar of the Milky Way was confirmed in 1991
(Blitz and Spergel) in almost the same orientation as I proposed.
(6) Yuan, C., "On the '3-kpc'
Arm: Resonance Excitation of Linear and non-linear Waves by an Oval
Distortion in the Central Region," Ap. J. 281, 600 (1984).
(SCI)
(7) Yuan, C., and Ye Cheng, "Resonance
Excitation: A Possible Interpretation of the 3-kpc Arm",
in The Outer Galaxy,
Ed. L. Blitz and J. Lochman, Springer-Verlag, 144-148 (1987).
4. Saturn's Rings and Proto-stellar Disks
Dr. Frank Shu and I developed a non-linear asymptotic theory of
resonance excitation and successfully applied it to the
interpretation of the structure of Saturn's rings. Extending the
theory for Saturn's Rings by including the stress tensor for pressure
and viscosity, I re-formulated the problem, and with Dr. Pat Cassen,
we applied the theory to the proto-stellar disk, to examine the
principal spiral modes which are excited resonantly by a giant proto-planet
in the disk and the consequences of the disk-planet interaction.
(8) F.H. Shu, Yuan, C., and J.J. Lissauer, "Non-Linear
Spiral Density Waves: an Inviscid Theory", Ap. J., 291,
356-376 (1985). (SCI)
(9) Yuan, C., and Pat Cassen, "Resonantly
Driven Non-linear Density Waves in Protostellar Disks",
Ap.J., 436, 338 (1994) (SCI)
5. Resonance Excitation and Spiral Structure
in the Galactic Central Regions
This is a first step of my long-term research to understand the
mechanism of fuelling AGNs and starburst rings in the galactic center.
I believe the bar-disk interaction plays the central role in this.
I use (1) the non-linear asymptotic theory to study the bar-driven
density waves in the gas-dust disk in galactic central regions,
(2) the wavelet analysis to probe the hidden spiral-bar structure
of the HST observations, and (3) the gasdynamic codes, which we
have developed, to study the evolution of disks driven by a rotating
bar potential. The main results are not published yet. But my early
work has sufficiently reflected this trend. They are:
(10) Yuan, C., and Chao-Lin Kuo, "Bar-driven
Spiral Density Waves in Gaseous Disks", Ap.J., 486,
750 (1997). (SCI)
(11) Chao-Lin Kuo and Yuan, C., "Resonantly
Excited Waves in Gaseous Disks: Asymptotic Theory vs. Numerical
Hydrodynamics", Ap.J., 512, 79 (1999). (SCI)
6. Kinetic Theory of Disk Systems
Uri Griv and I have made a systematic study of disk systems in
search for Landau type of instabilities. We took a different approach
from the rest: (1) to consider of local gradients of density and
mean dispersion velocities in addition to the differential rotation,
and (2) to carry out second order epicyclic approximation; thus
perturbation velocity squares are included. We found various instabilities
and a wide range of implications. In particular, spiral density
waves can be self-excited at the corotation in a wave-disk interaction.
Another important result is that the critical dispersion velocity
for disk instability is equal to 2 /
time Toomre's value.
(12) Griv, E., Yuan, C., & Gedalin, M., "Dynamics
of Disk-shaped Stellar System: Resonant self-excitation/Absorption
of Density Waves", MNRAS, 307, 1 (1999). (SCI)
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