Deep inside low-mass stars

摘要：

Low-mass stars exhibit,at all stages of their evolution,the signatures of complex physical processes that require challenging modeling beyond standard stellar theory. In this review,we recall the most striking observational evidences that probe the interaction and interdependence of various transport processes of chemicals and angular momentum in these objects. We then focus on the impact of atomic diffusion,large scale mixing due to rotation,and internal gravity waves on stellar properties on the main sequence and slightly beyond.

关键词： hydrodynamics instabilities-turbulence-waves-stars:abundances-stars:evolution stars:interiors-stars:rotation

作者: Corinne Charbonnel Suzanne Talon

作者单位: Geneva Observatory,University of Geneva,ch.Des Maillettes 51,1290 Versoix,Switzerland;Laboratoire d RQCHP,Département de physique,Université de Montréal,C.P.6128,succ.centre-ville,Montréal,Québec,H3C

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: 163-174

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）