Self-gravitating disc-like magnetic gas clouds

被引：7

作者：

Barker, DM ^{[1
]}

Mestel, L ^{[1
]}

机构：

[1] UNIV SUSSEX,CTR ASTRON,BRIGHTON BN1 9QH,E SUSSEX,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1996年 / 282卷 / 02期

关键词：

magnetic fields; stars; formation; ISM; clouds; molecules;

D O I：

10.1093/mnras/282.2.317

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Two topics of importance for the theory of star formation are illustrated by treatment in a disc-like geometry: (1) the evolution through differential flux diffusion of a gas cloud initially in magneto-gravitational equilibrium, leading to the collapse of a cloud core; and (2) the effect-of turbulent support on the cloud structure, especially on the topology of the magnetic field.

引用

页码：317 / 326

页数：10

共 14 条

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