Not all stars form in clusters - measuring the kinematics of OB associations with Gaia

It is often stated that star clusters are the fundamental units of star formation and that most (if not all) stars form in dense stellar clusters. In this monolithic formation scenario, low-density OB associations are formed from the expansion of gravitationally bound clusters following gas expulsio...

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Bibliographic Details
Main Authors: Ward, Jacob L. (Author) , Kruijssen, Diederik (Author)
Format: Article (Journal)
Language:English
Published: 15 January 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 475, Issue: 4, Pages: 5659-5676
ISSN:1365-2966
DOI:10.1093/mnras/sty117
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/sty117
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/475/4/5659/4810564
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Author Notes:Jacob L. Ward and J.M. Diederik Kruijssen
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Not all stars form in clusters - measuring the kinematics of OB associations with Gaia by Ward, Jacob L. (Author) , Kruijssen, Diederik (Author) ,


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