The Origin of the Stellar Mass Distribution and Multiplicity

Yueh Ning Lee*, Stella S.R. Offner, Patrick Hennebelle, Philippe André, Hans Zinnecker, Javier Ballesteros-Paredes, Shu ichiro Inutsuka, J. M.Diederik Kruijssen

*此作品的通信作者

研究成果: 雜誌貢獻回顧評介論文同行評審

8 引文 斯高帕斯(Scopus)

摘要

In this chapter, we review some historical understanding and recent advances on the Initial Mass Function (IMF) and the Core Mass Function (CMF), both in terms of observations and theories. We focus mostly on star formation in clustered environment since this is suggested by observations to be the dominant mode of star formation. The statistical properties and the fragmentation behaviour of turbulent gas is discussed, and we also discuss the formation of binaries and small multiple systems.

原文英語
文章編號70
期刊Space Science Reviews
216
發行號4
DOIs
出版狀態已發佈 - 2020 六月 1

ASJC Scopus subject areas

  • 天文和天體物理學
  • 空間與行星科學

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