Presentation Information
[C06-2-04]Growth of Massive Molecular Filament by Accretion Flows: Origin of Constant Width
*Daisei Abe1, Tsuyoshi Inoue2, Shu-ichiro Inutuska1 (1. Nagoya University (Japan), 2. Konan University (Japan))
Keywords:
magnetohydrodynamics,star-formation,shock wave
