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...
Saved in:
| Main Authors: | , |
|---|---|
| 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 |
| Author Notes: | Jacob L. Ward and J.M. Diederik Kruijssen |
Search Result 1
Not all stars form in clusters - measuring the kinematics of OB associations with Gaia
Article (Journal)
Chapter/Article
Online Resource