Program
| Tuesday December 10, 2019 | |
|---|---|
| ISM, Star formation, and other physical processes | |
| 09:00~09:30 | Invited What do we learn about galaxy formation from simulations with realistic feedback? Xiangcheng Ma (University of California, Berkeley) |
| 09:30~10:00 | Invited Arepo-MCRT: Monte Carlo radiation hydrodynamics on a moving mesh Aaron Smith (MIT Kavli Institute) |
| 10:00~10:15 | Correlation between Faraday rotation measure and X-ray flux of evolving galaxy clusters Alvina Yee Lian On (Mullard Space Science Laboratory, University College London) |
| 10:15~10:30 | The microphysics of galaxy formation and evolution: the role of cosmic rays Ellis Owen (NTHU) |
| 10:30~11:00 | Coffee Break |
| 11:00~11:30 | Invited Feedback, chemistry, and turbulence in the interstellar medium:
insights from small-scale simulations. Chia-Yu Hu (Max Planck Institute for Extraterrestrial Physics) |
| 11:30~12:00 | Invited Galaxy simulation with the evolution of grain size distribution Shohei Aoyama (Academia Sinica) |
| 12:00~12:15 | Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from Their Dark Matter Using A Machine Trained on Hydrodynamic Simulations Yongseok Jo (Seoul National University) |
| 12:15~12:30 | Radiation hydro simulations with VET Wun-Yi Chen (ASIAA/NTU) |
| 12:30~14:00 | Lunch |
| 14:00~14:30 | Invited Yueh-Ning Lee (NTNU) |
| 14:30~15:00 | Pop III Suprnovae feedback and the first galaxies Ken Chen (ASIAA) |
| 15:00~15:15 | Mass loss of Massive Stars and their Feedback Po-Sheng Ou (ASIAA/ NTU) |
| 15:15~15:30 | Radiative Feedback of the EMP Binaries Sung-Han Tsai (ASIAA) |
| 15:30~16:00 | Coffee Break |
| 16:00~17:00 | Discussion |
| 18:00~20:00 | Banquet: 欣葉日本料理 信義A11館 台北市松壽路11號5樓(新光三越信義店A11館) |
asiaa.sinica.edu.tw