Program

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Thursday February 8, 2018
08:30	Shuttle from Landis Inn Chuhu to Workshop Venue
09:00~09:15	Grain Alignment in the Ophiuchus Molecular Cloud Abstract Kate Pattle (National Tsing Hua University)
09:15~09:30	Can we trace magnetic fields via polarized infrared emission from PAHs? Abstract Thiem Hoang (KASI and UST)
09:30~09:45	Magnetic Field in Massive Protoclusters Abstract Vivien Chen (National Tsing Hua University)
Session IV: Simulations of B-fields and/or turbulence 2 (Chair: Enrique Vazquez-semadeni)
09:45~10:15	Invited Study of Magnetic fields with velocity gradients Abstract Alex Lazarian (University of Wisconsin-Madison)
10:15~10:30	Not turbulence nor magnetic fields: just global hierarchical collapse of clouds. Abstract Enrique Vazquez-Semadeni (IRyA UNAM)
10:30~11:00	Coffee Break
11:00~11:15	Turbulence, magnetic field, and thermodynamics: what determines the IMF? Abstract Yueh-Ning LEE (IPGP)
11:15~11:30	Energy balance between turbulence and gravity in simulations of molecular cloud fragmentation. Abstract Vianey Camacho (Instituto de Radioastronomía y Astrofísica UNAM)
11:30~12:00	Discussion (lead by Giles Novak)
12:00~13:15	Lunch
13:15~13:30	Non-ideal magnetic fields in protostar formation Abstract James Wurster (University of Exeter)
13:30~13:45	The link between Magnetic-field Orientation and Star Formation Rates: From a simulation prospective Abstract Zitan Guo (the Chinese University of Hong Kong)
13:45~14:00	The effect of photoionising feedback on star formation in isolated and colliding turbulent clouds Abstract Kazuhiro Shima (Hokkaido University)
14:00~14:15	Velocity Anisotropy in Self-gravitating Molecular Clouds Abstract Hongli Liu (The Chinese University of Hong Kong, HK)
14:15~14:30	The Effect of Magnetic Fields and Ambipolar Diffusion on the Column Density Probability Distribution Function in Molecular Clouds Abstract Sayantan Auddy (University of Western Ontario, Canada)
Session V: Observations of GMCs and filaments (Chair: Hans Zinnnecker)
14:30~15:00	Invited POLSTAR survey: Magnetic fields in Pristine to Cluster Forming Filaments Abstract Thushara Pillai (MPIfR)
15:00~15:30	Invited Magnetic fields and turbulence in the diffuse interstellar medium Abstract Edith Falgarone (Ecole Normale Supérieure and Observatoire de Paris)
15:30~16:00	Coffee Break
16:00~16:15	Turbulent Properties in Star-Forming Molecular Clouds: Molecular Line Mapping with High-Velocity Resolution Using TRAO Abstract Hyeong-Sik Yun (Kyung Hee University)
16:15~16:30	Pinched magnetic field in a massive and quiescent filament Abstract Tie Liu (EAO/JCMT, KASI)
16:30~17:00	Invited The Tai Chi in Star Formation Abstract Hua-bai Li (CUHK)
17:00~17:15	New Views on Turbulence: The Riddle of Gravitational Binding in the Disk and Center of the Milky Way Abstract Jens Kauffmann (Haystack Observatory, Massachusetts Institute of Technology)
17:15~17:30	What are we learning from the relative orientation between density structures and the magnetic field in molecular clouds? Abstract Juan Diego Soler (Max Planck Institute for Astronomy)
17:30~17:45	The Musca molecular cloud: An interstellar symphony Abstract Aris Tritsis (Research School of Astronomy and Astrophysics, Australian National University)