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Numerical simulation of a planet interacting with a protoplanetary disk (Zhang, Yuan and Yen, in preparation).
Numerical simulation of a planet interacting with a protoplanetary disk
Comparison between a numerical simulation result (left) and M81 (right). M81 is a well studied case of spiral stellar potential driven shock and star formation. The secondary spiral structure observed outside the main shock (bottom-right feature in the ri
omparison between a numerical simulation result and M81
Numerical simulation of the structure of NGC 1300 under a strong bar potential. The figures from left to right are the numerical result, observation, and their superposition, respectively.
Numerical simulation of the structure of NGC 1300 under a strong bar potential
Yuan, Chi
(passed away on July 24, 2008)
photo of Yuan, Chi
Email: n/a

Education and Positions

  • Distinguished Visiting Scholar, ASIAA (2007~2008)

Research Interests

Theoretical Astrophysics, Numerical Simulation of Galactic Dynamics

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