Vardya, M. S. (1984) Mass loss and R 136a-type stars Publications of the Astronomical Society of the Pacific, 96 (583). pp. 743-745. ISSN 0004-6280
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Official URL: http://www.jstor.org/pss/40678398
Related URL: http://dx.doi.org/10.1086/131414
Abstract
Empirical and semiempirical expressions for the rate of mass loss, derived for O and B stars, have been examined vis-a-vis R 136a. The best expression has been used to predict the rate of mass loss for some R 136a-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.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to University of Chicago Press. |
| Keywords: | Mass Loss; Massive Stars; H II Regions |
| ID Code: | 57467 |
| Deposited On: | 27 Aug 2011 15:13 |
| Last Modified: | 27 Aug 2011 15:13 |
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