Collapse of a molecular cloud core to stellar densities: stellar core and outflow formation in radiation magnetohydrodynamics simulations (vol 465,pr 2714,2017)

被引:0
作者
Bate, Matthew R. [1 ]
Tricco, Terrence S. [2 ]
Price, Daniel J. [2 ]
机构
[1] Univ Exeter, Sch Phys & Astron, Stocker Rd, Exeter EX4 4QL, Devon, England
[2] Monash Univ, Sch Math Sci, Monash Ctr Astrophys, Clayton, Vic 3800, Australia
关键词
accretion; accretion discs; MHD; radiative transfer; stars: evolution; stars: formation; stars: winds; outflows; SMOOTHED PARTICLE MAGNETOHYDRODYNAMICS;
D O I
10.1093/mnras/stw2940
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:2714 / 2716
页数:3
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