Thermohaline mixing and fossil magnetic fields in red giant stars
We discuss the occurence and consequences of thermohaline mixing in RGB stars,as well as the possible inhibition of this process by a fossil magnetic field in Ap star descendants.
hydrodynamics-instabilities-stars:abundances-stars:evolution-stars:interiors-stars:rotation
Corinne Charbonnel Jean-Paul Zahn
Geneva Observatory,University of Geneva,ch.Des Maillettes 51,1290 Versoix,Switzerland;Laboratoire d LUTH,Observatoire de Paris,CNRS,Université Paris-Diderot,France
国际会议
The 252th Symposium of the International Astronomical Union(国际天文学联合会第252届研讨会)
海南三亚
英文
245-246
2008-04-06(万方平台首次上网日期,不代表论文的发表时间)