The formation of massive stars : accretion , disks , and the development of hypercompact HII regions Eric Keto

Abstract

The hypothesis that massive stars form by accretion can be investigated by simple analytical calculations that describe the effect that the formation of a massive star has on its own accretion flow. Within a simple accretion model that includes angular momentum, that of gas flow on ballistic trajectories around a star, the increasing ionization of a massive… (More)

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@inproceedings{Keto2007TheFO, title={The formation of massive stars : accretion , disks , and the development of hypercompact HII regions Eric Keto}, author={Eric R. Keto}, year={2007} }