Other
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...326..208t&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 1, 1988, p. 208-222.
Other
53
Interstellar Gas, Magnetohydrodynamics, Nebulae, Star Formation, Stellar Rotation, Angular Momentum, Magnetic Fields, Mass Distribution, Self Consistent Fields
Scientific paper
It is shown that the equilibrium structure of a self-gravitating, magnetized, isothermal cloud with rotation can be solved by the self-consistent field method, like that employed in the pioneering work on a magnetized cloud without rotation by Mouschovious. Clouds are assumed to be axisymmetric and are embedded in a stationary external medium. The equilibrium problem is characterized by four free parameters; the central gas density, the total angular momentum, the total mass, and the magnetic flux. Two free functions, the distributions of specific angular momentum and mass within a cloud, should be given. These six quantities characterize each equilibrium model. Several numerical examples are shown.
Ikeuchi Satoru
Nakamura Takashi
Tomisaka Kohji
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