The equilibria and evolutions of magnetized, rotating, isothermal clouds. IV - Quasi-static evolution

Details The equilibria and evolutions of magnetized, rotating, isothermal clouds. IV - Quasi-static evolution The equilibria and evolutions of magnetized, rotating, isothermal clouds. IV - Quasi-static evolution

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...362..202t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 362, Oct. 10, 1990, p. 202-214.

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40

Interstellar Magnetic Fields, Magnetic Flux, Magnetohydrodynamic Waves, Molecular Clouds, Plasma Drift, Rotating Fluids, Angular Momentum, Isothermal Flow, Star Formation, Zeeman Effect

Scientific paper

The evolution of a rotating magnetized cloud is studied using a numerical method and a quasi-static assumption. The angular momentum loss rate is discussed, including the critical value of the mass-to-flux ratio at which point the cloud begins to collapse dynamically. The difference between the present case and a plane-parallel cloud is examined.

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