Surface convection in Population Ⅱ stars
The initial surface abundances of Population Ⅱ stars have been altered by the interplay between convection,rotational mixing and diffusion. In particular the shallower the outer convection zone the stronger the diffusion impact. We present preliminary results on constraining the extension of the convection zones of Population Ⅱ stars thanks to 3D hydrodynamical simulations.
Convection stars:populations Ⅱ
Laurent Piau Robert F.Stein
CEA-Saclay DSM/IRFU/SAp,LOrme des Merisiers 91191 Gif-sur-Yvette France Michigan State University,Department of Physics & Astronomy East Lansing,MI 48824-2320,USA
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
253-254
2008-04-06(万方平台首次上网日期,不代表论文的发表时间)