Massive star formation by accretion: II. Rotation: how to circumvent the angular momentum barrier?
<i>Context. <i/>Rotation plays a key role in the star-formation process, from pre-stellar cores to pre-main-sequence (PMS) objects. Understanding the formation of massive stars requires taking into account the accretion of angular momentum during their PMS phase.<i>Aims. <i/>...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
24 May 2017
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| In: |
Astronomy and astrophysics
Year: 2017, Jahrgang: 602 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201630149 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201630149
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| Verfasserangaben: | L. Haemmerlé, P. Eggenberger, G. Meynet, A. Maeder, C. Charbonnel, and R.S. Klessen |
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Massive star formation by accretion: II. Rotation: how to circumvent the angular momentum barrier?
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