Thermal-convective-instability of a stellar atmosphere in the presence of a nonlinear magnetic field

Details Thermal-convective-instability of a stellar atmosphere in the presence of a nonlinear magnetic field Thermal-convective-instability of a stellar atmosphere in the presence of a nonlinear magnetic field

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.196..109a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 196, no. 1, p. 109-115.

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Stellar Atmospheres, Stellar Magnetic Fields, Thermal Instability, Free Convection, Nonlinear Equations, Stellar Rotation

Scientific paper

Thermal-convective-instability of a stellar atmosphere is investigated in the presence of a nonlinear magnetic field. A model proposed by Roberts (1981) in the context of neutron stars is used. The simultaneous effect of both nonlinear magnetic field and rotation is also considered. The criteria obtained for monotonic instability generalize the criterion derived by Defouw (1970) in the absence of magnetic field and rotation.

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