A quantitative study of O stars in NGC 2244 and the Monoceros OB2 association

Type: Article

Publication Date: 2011-11-16

Citations: 78

DOI: https://doi.org/10.1051/0004-6361/201117458

Abstract

Aims. Our goal is to determine the stellar and wind properties of seven O stars in the cluster NGC 2244 and three O stars in the OB association Mon OB2. These properties give us insight into the mass loss rates of O stars. They allow us to both check the validity of rotational mixing in massive stars and to better understand the effects of the ionizing flux and wind mechanical energy release on the surrounding interstellar medium and its influence on triggered star formation.

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  • Astronomy and Astrophysics - View - PDF
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