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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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
15 January 2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 475, Heft: 4, Pages: 5659-5676 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty117 |
| Online-Zugang: | 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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| Verfasserangaben: | 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
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