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Pitfalls when observationally characterizing the relative formation rates of stars and stellar clusters in galaxies

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Stars generally form in aggregates, some of which are bound (‘clusters’) while others are unbound and disperse on short ($${\sim }10 {\,{\rm Myr}}$$) time-scales (‘associations’). The fraction of stars forming in bound clusters (Γ) is a fundamental outcome of the star formation process. Recent obser...

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Bibliographic Details
Main Authors: Kruijssen, Diederik (Author) , Bastian, Nate (Author)
Format: Article (Journal)
Language:English
Published: 05 January 2016
In: Monthly notices of the Royal Astronomical Society. Letters
Year: 2016, Volume: 457, Issue: 1, Pages: L24-L28
ISSN:1745-3933
DOI:10.1093/mnrasl/slv182
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnrasl/slv182
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Author Notes:J. M. Diederik Kruijssen and Nate Bastian
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Pitfalls when observationally characterizing the relative formation rates of stars and stellar clusters in galaxies by Kruijssen, Diederik (Author) , Bastian, Nate (Author) ,


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