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球状星団M30の2つの異なる青い落とし星のシーケンス

F R Ferraro1, G Beccari, E Dalessandro

  • 1Department of Astronomy, University of Bologna, Via Ranzani 1, 40127 Bologna, Italy. francesco.ferraro3@unibo.it

Nature
|December 25, 2009
PubMed
まとめ

M30球状星団の2つの異なる青い落とし星集団は,異なる形成経路を示唆しています. 核の崩壊は,星衝突と二重質量移転の両方を強化し,2つのユニークなブルー・ストラグラー・シーケンスを作成した.

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