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Magnetic fields of OB stars

Published online by Cambridge University Press:  07 August 2014

A. F. Kholtygin
Affiliation:
Saint Petersburg State University, Universitetski pr. 28, Petrodvorets, 198504, Saint Petersburg, Russia, email: afx-afx@mail.ru
S. Hubrig
Affiliation:
Leibniz-Institut für Astrophysik, Potsdam, Germany, email: shubrig@aip.de
N. A. Drake
Affiliation:
Saint Petersburg State University, Universitetski pr. 28, Petrodvorets, 198504, Saint Petersburg, Russia, email: afx-afx@mail.ru Observatório Nacional/MCTI, Rua General José Cristino 77, 20921-400, Rio de Janeiro, Brazil, email: drake@on.br
N. Sudnik
Affiliation:
Saint Petersburg State University, Universitetski pr. 28, Petrodvorets, 198504, Saint Petersburg, Russia, email: afx-afx@mail.ru
V. Dushin
Affiliation:
Saint Petersburg State University, Universitetski pr. 28, Petrodvorets, 198504, Saint Petersburg, Russia, email: afx-afx@mail.ru
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Abstract

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We studied the statistical properties of the magnetic fields of OB stars based on the recent measurements. As the statistically significant characteristic of the magnetic field we use the rms magnetic field of the star ${\cal B}$. The distribution functions f(${\cal B}$) of magnetic fields of OB stars are evaluated. The function f(${\cal B}$) has a power-law dependence on the ${\cal B}$ with an index of about 2-3 and a fast drop below ${\cal B}$ = 100 − 300 G. We proposed that the compact regions with strong local magnetic fields can contribute to the global magnetic field of O stars.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

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