Massive star formation by accretion: II. Rotation: how to circumvent the angular momentum barrier?
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. We study the PMS evolution of objects destined to be...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
March 27, 2017
|
| In: |
Arxiv
|
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1703.08357
|
| Verfasserangaben: | L. Haemmerlé, P. Eggenberger, G. Meynet, A. Maeder, C. Charbonnel, R.S. Klessen |
Search Result 1