A Model for Adiabatic Mass-loss

摘要：

We describe our work on the development and application of a stellar structure code to compute model sequences representing donor stars in interacting binaries subject to rapid (adiabatic) mass-loss. The donor star is assumed to remain in hydrostatic equilibrium,but no heat flow is allowed. These sequences can be used to define bifurcation sequences in close binary evolution,and to circumscribe possible survivors of common envelope evolution.

关键词： stars:evolution stars:interiors stars:mass loss binaries:close

作者: Hongwei.Ge R.F.Webbink Z.Han

作者单位: National Astronomical Observatories/Yunnan Observatory,Chinese Academy of Sciences,Kunming 650011,Ch Department of Astronomy,University of Illinois,1002 W.Green St.Urbana,IL 61801,USA National Astronomical Observatories/Yunnan Observatory,Chinese Academy of Sciences,Kunming 650011,Ch

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: 419-420

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）