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