SPH with radiative transfer: Method and applications

被引:0
作者
Bastien, P [1 ]
Cha, SH [1 ]
Viau, S [1 ]
机构
[1] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada
来源
GRAVITATIONAL COLLAPSE: FROM MASSIVE STARS TO PLANETS | 2004年 / 22卷
关键词
methods : numerical; stars : formation;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An implicit method for radiative transfer in SPH is described. The diffusion approximation is used in this method, and the hydrodynamic calculations are performed by a fully three-dimensional SPH code. Various energy states and the dissociation of hydrogen molecules are considered in the energy calculation for a more realistic temperature determination. We have performed non-isothermal collapse simulations of a centrally condensed cloud, and have compared with the results of finite difference calculations performed by Myhill & Boss (1993). The results produced by the two completely different numerical methods agree well with each other. We also perform a rotating cylindrical cloud collapse to investigate the formation and evolution of disks, and present some results.
引用
收藏
页码:144 / 147
页数:4
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