The accretion history of high-mass stars: an ArTéMiS pilot study of infrared dark clouds
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DOI: 10.1093/mnras/staa1656
Abstract: The mass growth of protostars is a central element to the determination of fundamental stellar population properties such as the initial mass function. Constraining the accretion history of individual protostars is therefore an important aspect… read more here.
Keywords: mass stars; accretion history; high mass; mass ... See more keywords