Magnetic Fields and the Formation of Cores and Disks

被引:0
|
作者
Basu, Shantanu [1 ]
Bailey, Nicole D. [1 ]
Dapp, Wolf B. [2 ]
机构
[1] Univ Western Ontario, Dept Phys & Astron, London, ON N6A 3K7, Canada
[2] FZ Julich, Inst Adv Simulat, Julich Supercomp Ctr, Julich, Germany
来源
NEW TRENDS IN RADIO ASTRONOMY IN THE ALMA ERA: THE 30TH ANNIVERSARY OF NOBEYAMA RADIO OBSERVATORY | 2013年 / 476卷
关键词
HYDROMAGNETIC WAVE SUPPORT; STRATIFIED MOLECULAR CLOUD; AMBIPOLAR DIFFUSION; MILKY-WAY; SIMULATIONS; COLLAPSE; OBJECTS; BRAKING;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We review recent results of non-ideal magnetohydrodynamic models for the fragmentation of molecular clouds and the collapse of cloud cores to form protostar-disk systems. Thin-disk models can elucidate many aspects of the physical problem and allow the calculation of large dynamic range of time and length scales.
引用
收藏
页码:103 / 110
页数:8
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