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The Origin of the Stellar Mass Distribution and Multiplicity

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.

preprint2020arXivOpen access
Yueh-Ning LeeStella S. R. OffnerPatrick HennebellePhilippe AndréHans ZinneckerJavier Ballesteros-ParedesShu-ichiro InutsukaJ. M. Diederik Kruijssen
astro-ph.GA
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Open access8 authors1 topic
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Yueh-Ning LeeStella S. R. OffnerPatrick HennebellePhilippe AndréHans ZinneckerJavier Ballesteros-ParedesShu-ichiro InutsukaJ. M. Diederik Kruijssen

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