Mass loss and R 136a-type stars

Details Mass loss and R 136a-type stars Mass loss and R 136a-type stars

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..743v&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, Sept. 1984, p. 743-745.

Astronomy and Astrophysics

Astronomy

B Stars, Hydrogen Clouds, O Stars, Stellar Mass Ejection, Giant Stars, Star Clusters

Scientific paper

Empirical and semiempirical expressions for the rate of mass loss, derived for O and B stars, have been examined vis-a-vis R136a. The best expression has been used to predict the rate of mass loss for some R136a-type objects. The change in predicted values, when these objects are not single stars but are composed of a dense cluster of similar stars has been discussed.

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