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The Rise of a Magnetic Flux Tube through the Radiative Envelope of a 9 M⊙ Star

Published online by Cambridge University Press:  12 April 2016

J. P. Cassinelli  and
K. B. MacGrego
J. P. Cassinelli
Affiliation:
NCAR, High Altitude Observatory, Boulder, CO 80307-3000 Astronomy Department, University of Wisconsin, Madison, WI 53706-1582
K. B. MacGrego
Affiliation:
NCAR, High Altitude Observatory, Boulder, CO 80307-3000

Abstract

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We explore the possibility that the magnetic field generated by a dynamo at the interface between the convective core and radiative envelope of a massive star can be transported to the surface by buoyancy.

Type
4. Aperiodic Variations
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 337 - 343
Copyright
Copyright © Astronomical Society of the Pacific 2000

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