Internal motions in magnetic stars

Details Internal motions in magnetic stars Internal motions in magnetic stars

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196..491n&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 196, Aug. 1981, p. 491-506. Research supported by the British Council.

Astronomy and Astrophysics

Astronomy

17

Convective Flow, Magnetic Field Configurations, Magnetic Stars, Stellar Interiors, Stellar Rotation, Stellar Structure, A Stars, Blue Stars, Mass Flow Rate, Nutation, Stellar Envelopes, Stellar Magnetic Fields, Stellar Mass, Stellar Models, Stellar Motions

Scientific paper

The dynamically driven, adiabatic, internal motions for an obliquely rotating magnetic star are estimated for the case where the toroidal component of the magnetic field dominates. The consequent mixing due to these motions is discussed in relation to: (1) the diffusion theory for the Ap phenomena, and (2) the blue straggler stars. Also, the behavior of the time-scales for the obliquity angle to reach its asymptotic state is reported for a range of stellar masses for stars with either dominant poloidal or toroidal magnetic fields.

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