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Magnetic Fields in Be Stars? (Review Paper)

Published online by Cambridge University Press:  23 September 2016

Paul K. Barker
Paul K. Barker*
Affiliation:
Astronomy Department, University of Western Ontario, London, Ontario N6A 3K7, Canada

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., Brown, D.N. & Marlborough, J.M. (1987). In preparation.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. (1979). Ap. J., 228, 809.Google Scholar
Borra, E.F., Landstreet, J.D., & Mestel, L. (1982). Ann. Rev. Astron. Astrophys., 20, 191.CrossRefGoogle Scholar
Crampin, J., & Hoyle, F. (1960). M.N.R.A.S., 120, 33.Google Scholar
Gnedin, Y.N., & Silant'ev, N.A. (1984). Astrophys. & Space Science, 102, 375.Google Scholar
Groote, D., & Hunger, K. (1982). Astr. Ap., 116, 64.Google Scholar
Hazlehurst, J. (1967). Zs. fur Ap., 65, 311.Google Scholar
Henriksen, R.N. (1969). Astr. Ap., 1, 457.Google Scholar
Landstreet, J.D. (1980). A.J., 85, 611.CrossRefGoogle Scholar
Landstreet, J.D. (1982). Ap. J., 258, 639.CrossRefGoogle Scholar
Landstreet, J.D., & Borra, E.F. (1978). Ap. J. (Letters), 224, L5.Google Scholar
Limber, D.N. (1974). Ap. J., 192, 429.Google Scholar
Limber, D.N., & Marlborough, J.M. (1968). Ap. J., 152, 181.CrossRefGoogle Scholar
Mestel, L., & Moss, D.L. (1983). M.N.R.A.S., 204, 575.Google Scholar
Mihalas, D., & Conti, P.S. (1980). Ap. J., 235, 515.Google Scholar
Moss, D. (1980). Astr. Ap., 91, 319.Google Scholar
Nakajima, R. (1981). Science Reports of the Tohoku University, 8th Series, 2, No. 3, p. 130.Google Scholar
Nerney, S. (1980). Ap. J., 242, 723.Google Scholar
Poe, C.H., & Friend, D.B. (1986). Ap. J., in press.Google Scholar
Saito, M. (1974). Pub. Astr. Soc. Japan, 26, 103.Google Scholar
Saito, M., & Saito, Y. (1984). Pub. Astr. Soc. Japan, 36, 603.Google Scholar
Severny, A. (1970). Ap. J. (Letters), 159, L73.Google Scholar
Strittmatter, P.A., & Norris, J. (1971). Astr. Ap., 15, 239.Google Scholar
Thompson, I.B., & Landstreet, J.D. (1985). Ap. J. (Letters), 289, L9.CrossRefGoogle Scholar
Underhill, A.B. (1984). Ap. J., 276, 583.Google Scholar
Underhill, A.B., & Fahey, R.P. (1984). Ap. J., 280, 712.Google Scholar
Weber, E.J., & Davis, L.D. (1967). Ap. J., 148, 217.Google Scholar