NLTE analysis of massive OB stars in open clusters

Bibcode
1990Ap&SS.169....7H
DOI
10.1007/BF00640677
Herrero, A.; Kudritzki, R. P.; Vilchez, J. M.
Bibliographical reference

IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989 Astrophysics and Space Science (ISSN 0004-640X), vol. 169, no. 1-2, July 1990, p. 7-13.

Advertised on:
7
1990
Number of authors
3
IAC number of authors
0
Citations
1
Refereed citations
1
Description
The paper presents a new method for deriving stellar masses and distances using the theory of radiatively driven winds as presented by Kudritzki et al. (1989) and the stellar parameters derived from NLTE spectroscopic analysis. The procedure is illustrated with five stars observed in three open clusters. Comparison with evolutionary tracks indicates a possible discrepancy between the masses and helium abundances (when enhanced) derived from these tracks and those obtained by other methods.
Type
Non-refereed
B stars
O stars
Stellar evolution
Stellar winds

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