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Magnetic Fields in Be Stars? (Review Paper)
Published online by Cambridge University Press: 23 September 2016
Abstract
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No mean longitudinal or toroidal magnetic fields have yet been detected on any classical Be star. Models of stellar winds and circumstellar envelopes around magnetic Be stars are not appreciably constrained by present observed upper limits on field strength. A few magnetic Be stars do exist among the helium strong stars, but these objects show spectral phenomenology which is unmistakably distinct from that shown by every other object known as a Be star.
- Type
- IIA. The Underlying Stars: Observations
- Information
- International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 38 - 48
- Copyright
- Copyright © Cambridge University Press 1987
References
Barker, P.K. (1987) In IAU Colloquium 87, Hydrogen Deficient Stars and Related Objects (Dordrecht: Reidel), in press.Google Scholar
Barker, P.K., Bolton, C.T., Brown, D.N., Landstreet, J.D., & Shore, S.N. (1987) In preparation.Google Scholar
Barker, P.K., Brown, D.N., Bolton, C.T., & Landstreet, J.D. (1982). NASA Conference Publication CP-2238, p. 589.Google Scholar
Barker, P.K., Landstreet, J.D., Marlborough, J.M., & Thompson, I.B. (1985). Ap. J., 288, 741.Google Scholar
Barker, P.K., Landstreet, J.D., Marlborough, J.M., Thompson, I.B., & Maza, J. (1981). Ap. J., 250, 300.Google Scholar
Borra, E.F., Landstreet, J.D., & Mestel, L. (1982). Ann. Rev. Astron. Astrophys., 20, 191.CrossRefGoogle Scholar
Nakajima, R. (1981). Science Reports of the Tohoku University, 8th Series, 2, No. 3, p. 130.Google Scholar
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