根据轨道根数探讨特殊红巨双星的形成机制  

Insights into Formation of Chemical Peculiar Red Gianta from Orbital Elements

作　　者：刘俊红[1] 刘澎洲 张会芳[3] 

机构地区：[1]石家庄学院物理系,河北石家庄050035 [2]河北晋州实验中学,河北晋州052260 [3]石家庄学院图书馆,河北石家庄050035

出　　处：《石家庄学院学报》2009年第6期5-8,共4页Journal of Shijiazhuang University

摘　　要：比较了普通红巨双星与特殊红巨星轨道根数的特性,讨论了各类特殊红巨双星系统质量传输的途径,解释了特殊红巨星的形成机制.Based on the comparison between normal red binary giants and peculiar red binary giants in the feature of orbital elements,this paper deals with scenario of mass transfer for various families chemically-peculiar red giants binary systems,explaining formation of chemical peculiar red giants.

关 键 词：特殊红巨星 星风吸积 洛希瓣充满(RLOF) 公共包层抛射 

分 类 号：P142.9[天文地球—天体物理]