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Updated: May 5, 2026

Bringing the Visible Universe into Focus with Robo-AO
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青い恒星物体M17-SO1のシルエットには高質量原星はありません

Shigeyuki Sako1, Takuya Yamashita, Hirokazu Kataza

  • 1Department of Astronomy, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan. sako@ioa.s.u-tokyo.ac.jp

Nature
|April 23, 2005
PubMed
まとめ

巨大な恒星の形成は不明である. この研究は,主張された巨大な原星の発見を修正し,それが中間質量であることが判明し,高質量星の単一星形成理論に挑戦しています.

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