Impact of initial models and variable accretion rates on the pre-main-sequence evolution of massive and intermediate-mass stars and the early evolution of H II regions
Abstract. Massive star formation requires the accretion of gas at high rate while the star is already bright. Its actual luminosity depends sensitively on the
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2016 February 29
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2016, Jahrgang: 458, Heft: 3, Pages: 3299-3313 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw517 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stw517 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/458/3/3299/2589347 
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| Verfasserangaben: | Lionel Haemmerlé and Thomas Peters |
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