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Magnetic fluxes of massive stars: statistics and evolution

Published online by Cambridge University Press:  12 July 2011

Alexander F. Kholtygin ,
Sergei N. Fabrika ,
Natalia A. Drake  and
Andrei P. Igoshev
Alexander F. Kholtygin
Affiliation:
Astronomical Instituut, Saint-Petersburg University, 198504, ul Shaxmatova, Petrodvoretz, Rissia email: [email protected]
Sergei N. Fabrika
Affiliation:
Special Astrophysical Observatoty, Nizhnii Arxyz, Russia
Natalia A. Drake
Affiliation:
Astronomical Instituut, Saint-Petersburg University, 198504, ul Shaxmatova, Petrodvoretz, Rissia email: [email protected]
Andrei P. Igoshev
Affiliation:
Astronomical Instituut, Saint-Petersburg University, 198504, ul Shaxmatova, Petrodvoretz, Rissia email: [email protected]
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Abstract

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The statistical properties of magnetic fields and magnetic fluxes of OB stars were investigated. The mean magnetic fluxes of massive OB stars appear to be 3 order larger than those for neutron stars.

Keywords

stars: early-typestars: magnetic fieldsstars: neutron
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 198 - 199
Copyright
Copyright © International Astronomical Union 2011

References

Bychkov, V. D., Bychkova, L. V., & Madej, J. 2009, MNRAS, 394, 1338CrossRefGoogle Scholar
Aurière, M., Wade, G. A., Silvester, J., Lignières, F. et al. 2007, A&A, 475, 1053Google Scholar
Kholtygin, A. F., Fabrika, S. N., Drake, N. A., Bychkov, V. D. et al. 2010a, Astron. Lett., 36, 370CrossRefGoogle Scholar
Kholtygin, A. F., Fabrika, S. N., Drake, N. A., Bychkov, V. D. et al. 2010b, Kinematics and Physics of Celestial Bodies, 26, 181CrossRefGoogle Scholar