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On the Possible Role of Magnetic Fields in the Dynamics of the Be Phenomenon

Published online by Cambridge University Press:  14 August 2015

D. Nelson Limber
D. Nelson Limber*
Affiliation:
Dept. of Astronomy, University of Virginia, Charlottesville, Va., U.S.A.

Extract

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A problem that has intrigued me for some years is that of the dynamics of the Be phenomenon. For, although the Be phenomenon has been extensively studied for decades, the problems associated with the dynamics of the circumstellar envelopes about Be stars - the problems associated with their formation, with their maintenance, and with their dissolution - have, until very recently, received little more than qualitative consideration.

Type
Part V: Models
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 371 - 373
Copyright
Copyright © Reidel 1976 

References

Leighton, R. B.: 1969, Astrophys. J. 156, 1.CrossRefGoogle Scholar
Limber, D. N.: 1974, Astrophys. J. 192, 429.CrossRefGoogle Scholar
Marlborough, J. M. and Zamir, M.: 1975, Astrophys. J. 195, 145.CrossRefGoogle Scholar