The influence of inhomogeneities on hot star wind model predictions

摘要：

We study the effect of wind inhomogeneities (clumping) on O star wind model predictions. For this purpose we artificially include clumping into our stationary NLTE wind models. As a result of the inclusion of optically thin clumps the radiative line force is increased compared to corresponding unclumped models,with a similar effect on either the mass-loss rate or the terminal velocity. When the clumps are allowed to be optically thick in continuum,on the other hand,the radiative force and consequently the mass-loss rate decreases alternatively.

关键词： Stars:mass loss stars:early-type hydrodynamics

作者: J.Krti(c)ka L.Muijres J.Puls J.Kubāt A.de Koter

作者单位: Institute of Theoretical Physics and Astrophysics,Masaryk University,Brno,Czech Republic Astronomical Institute,Anton Pannekoek,University of Amsterdam,Amsterdam,The Netherlands Universit(a)tssternwarte München,München,Germany Astronomick(y) ustav,Ond(r)ejov,Czech Republic

会议类型: 国际会议

会议名称: The 252th Symposium of the International Astronomical Union(国际天文学联合会第252届研讨会)

会议地点: 海南三亚

会议语种:英文

页码: 283-288

在线出版日期: 2008-04-06（万方平台首次上网日期，不代表论文的发表时间）