Protostellar collapse with RHD in spherical symmetry

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概要

• 論文の詳細を見る

• We present a numerical radiation hydrodynamic calculation in multifrequency applied to the protostellar collapse. The past works which calculated collapse of protostellar clouds were based on the assumptions such as isothermal condition, the diffusion approximation and/or the grey approximation. On the contrary, our calculation requires none of them. As a test case, we calculated the collapse of a 1M_o homogeneous cloud.

• 素粒子論グループ 素粒子研究編集部の論文
• 1996-06-20

著者

• 増永 浩彦

  天文台

• MIYAMA Shoken

  Division of Theoretical Astrophysics, National Astronomical Observatory

• Miyama Shoken

  Division Of Theoretical Astrophysics National Astronomical Observatory

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• Protostellar collapse with RHD in spherical symmetry

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