The stability of magnetohydrodynamic stellar winds

Details The stability of magnetohydrodynamic stellar winds The stability of magnetohydrodynamic stellar winds

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..145s&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Stellar Winds: Magnetohydrodynamics

Scientific paper

Magnetohydrodynamic winds flowing out from fast-rotating stars are
analyzed. Acceleration of the winds is briefly discussed with relation
to the location of the singular points of the basic equations. The local
stabilities of the winds are examined.

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