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巨大な恒星形成のために,コラムの最小密度は1gcm(-2) です

Mark R Krumholz1, Christopher F McKee

  • 1Astrophysics Department, Princeton University, Princeton, New Jersey 08544, USA. krumholz@astro.princeton.edu

Nature
|February 29, 2008
PubMed
まとめ

巨大な恒星は,高密度の柱 (少なくとも1gcm−2) のガス雲で形成され,断片化を防ぐ. この値は,巨大な恒星が形成される場所を説明し,銀河全体の恒星形成率の変動を暗示しています.

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