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

页码：103 / 110

页数：8

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