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初期型銀河における恒星の初期質量関数の体系的な変化

Michele Cappellari1, Richard M McDermid, Katherine Alatalo

  • 1Department of Physics, University of Oxford, Oxford OX1 3RH, UK. cappellari@astro.ox.ac.uk

Nature
|April 28, 2012
PubMed
まとめ

恒星の初期質量関数 (IMF) は銀河ごとに大きく変化し,銀河の進化に影響を与えます. この研究は,IMFの差異が銀河質量と相関していることを明らかにし,形成の歴史が恒星群を形作ることを示唆しています.

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