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
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| Main Authors: | , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
2016 February 29
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2016, Volume: 458, Issue: 3, Pages: 3299-3313 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw517 |
| Online Access: | 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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| Author Notes: | Lionel Haemmerlé and Thomas Peters |
| Summary: | 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 |
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| Item Description: | Gesehen am 04.09.2020 |
| Physical Description: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw517 |