Final Presentations
| Last Updated: August 25, 2022 | |||||
|---|---|---|---|---|---|
| 29 Aug (Mon) | |||||
| Time | Place | Presentation | Supervisor | ||
| 10:30~10:50 | (remote) | Garvit Agarwal Investigating the impact of the single-moon assumption in exomoon modeling |
Alex Teachey | ||
| 10:50~11:10 | R1203 | Zhong-han Ai 艾宗瀚 Velocity Structures of ALMASOP Outflows |
Hsien Shang | ||
| 11:10~11:30 | R1203 | Yung-Ching Sun 孫詠晴 Explorations of Fourier Transform Algorithms |
Hsien Shang | ||
| 11:30~11:50 | R1203 | Cheng-Han Lai 賴政翰 Explorations of Murchison Meteorite Samples with X-ray Tomography using Synchrotron Radiation |
Hsien Shang | ||
| 14:20~14:40 | (remote) | Dionysios Gakis Investigating environment effects in the Saraswati supercluster |
Rogerio Monteiro-Oliveira | ||
| 14:40~15:00 | R1203 | Sy-Yun Pu 蒲思云 Constraining cosmological models with anisotropic clustering of halos in redshift space at high redshifts |
Teppei Okumura & Chian-Chou Chen | ||
| 15:20~15:40 | R1203 | Jo-Shui Kao 高若水 Fragmentation and properties of dense cores |
Hsi-Wei Yen | ||
| 15:40~16:00 | (remote) | Wing-Yu Siu 蕭詠輿 How are orbits of planets determined? |
Christian Flores Gonzalez & Nagayoshi Ohashi | ||
| 30 Aug (Tue) | |||||
| Time | Place | Presentation | Supervisor | ||
| 10:30~10:50 | (remote) | Van Le Planet-induced vortices with Disc Winds |
Michael Hammer | ||
| 10:50~11:10 | R1203 | Yung-Jiun Chen 陳永濬 Multi-Scale and Multi-Physics Hydro Simulations I. Superluminous Supernovae |
Ken Chen | ||
| 11:10~11:30 | R1203 | HsiangYu Chen 陳庠宇 Multi-Scale and Multi-Physics Cosmological Simulations -- Formation of Baby Galaxies |
Ken Chen | ||
| 11:30~11:50 | R1203 | Tsung-Han Chuang 莊宗翰 Molecular Gas Conditions in The Cores Before and After Onset of Star Formation |
Naomi Hirano | ||
| 14:00~14:20 | R1203 | Chia-Ming Chang 張家銘 Measuring the Gas Properties in LMC Superbubble DEM192 |
You-Hua Chu & Ting-Wen Lan | ||
| 14:20~14:40 | R1203 | Yining Huang 黃羿寧 Ultraviolet Observation of the Superbubble DEM 229 in the LMC |
You-Hua Chu & Ting-Wen Lan | ||
| 14:40~15:00 | (remote) | Vladislav Makeev Can multi-scale gas flows explain why the giant molecular filament G214.5-1.8 is so bad at forming stars? |
Seamus Clarke | ||
| 15:20~15:40 | R1203 | Ting-Xuan Li 李廷軒 Mass-Velocity Dispersion Relation in BAHAMAS Simulated Galaxy Clusters |
Sut leng Tam & Keiichi Umetsu | ||
| 15:40~16:00 | (remote) | Yinhao Wu 吴寅昊 Study the Hall Effect on Streaming Instability in Dusty Protoplanetary Disks |
Min-Kai Lin | ||
| 16:00~16:20 | R1203 | Ya-Chi Wang 王亞琪 Particle acceleration in hydrodynamic shocks |
Kouichi Hirotani & Hsien Shang | ||
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