Stability of the System of Stars, Gas, and Magnetic Fields

Details Stability of the System of Stars, Gas, and Magnetic Fields Stability of the System of Stars, Gas, and Magnetic Fields

Feb 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970ap%26ss...6..297n&link_type=abstract

Astrophysics and Space Science, Volume 6, Issue 2, pp.297-314

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Linear stability of a system of stars, gas and magnetic fields under the existence of a relative motion between the stars and the gas is investigated by the use of the magnetohydrodynamic and the polytropic equations for the gas and the collisionless Boltzmann equation for the stars together with the Poisson equation. The star system is supposed to have the anisotropic Schwarzschild distribution. The critical wavenumber is calculated and it is found that the system becomes universally unstable under some conditions.

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