Self-gravitating disc-like magnetic gas clouds

Details Self-gravitating disc-like magnetic gas clouds Self-gravitating disc-like magnetic gas clouds

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.282..317b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 282, Issue 2, pp. 317-326.

Astronomy and Astrophysics

Astronomy

7

Magnetic Fields, Stars: Formation, Ism: Clouds, Ism: Molecules

Scientific paper

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.

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