Wolf-Rayet stars - Physical, chemical and mass loss properties and evolutionary status

被引:8
作者
Willis, AJ
机构
[1] Department of Physics and Astronomy, University College London, London WC1E 6BT, Gower Street
关键词
D O I
10.1007/BF02424430
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper reviews the current status of knowledge regarding the basic physical and chemical properties of Wolf-Rayet stars; their overall mass loss and stellar wind characteristics and current ideas about their evolutionary status. WR stars are believed to be the evolved descendents of massive O-type stars, in which extensive mass loss reveals successive stages of nuclear processed material: WN stars the products of interior CNO-cycle hydrogen burning, and WC and WO stars the products of interior helium burning. Recent stellar evolution models, particularly those incorporating internal mixing, predict results which are in good accord with the different chemical compositions observationally inferred for WN, WC and WO stars. WR stars exhibit the highest levels of mass loss amongst early type stars: mass loss rates, typically, lie in the range [1-10] x 10(-5) M(.)yr(-1). Radiation pressure-driven winds incorporating multi-scattering in high ionisation-stratified winds may cause these levels, but additional mechanisms may also be needed.
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收藏
页码:145 / 168
页数:24
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