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Parameters of the average magnetic phase curves

Published online by Cambridge University Press:  02 March 2005

V.D. Bychkov ,
L.V. Bychkova  and
J. Madej
V.D. Bychkov
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Russia email: vbych@sao.ru
L.V. Bychkova
Affiliation:
Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Russia email: vbych@sao.ru
J. Madej
Affiliation:
Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland email: jm@alkor.astrouw.edu.pl Present address: SAO RAS, Nizhni Arkhyz, 369167 Russia.
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Abstract

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We analyse parameters of the average phase curves of the effective magnetic field $B_{\rm e}$ for 139 Main Sequence and other stars. 134 are chemically peculiar A and B type stars. This contribution presents the statistical properties of the fitting coefficients $B_{\rm 0}$, $B_{\rm 1}$, and $B_{\rm 2}$, and the distribution of the parameter $r= B_{\rm e}({\rm max})/B_{\rm e}({\rm min})$.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Magnetic starsmagnetic variability
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 642 - 646
Copyright
© 2004 International Astronomical Union