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Magnetic configurations of the fast CP rotators HD3360, HD4778, HD5737, HD112413, and HD215441

Magnetic configurations of the fast CP rotators HD3360, HD4778, HD5737, HD112413, and HD215441 The method of “magnetic charges” is used to model magnetic fields of five rapidly rotating stars (P < 25d) and to find the basic parameters of their magnetic fields. A table containing all the modeling results obtained using the adopted method as well as the parameters obtained for the same stars by other authors is presented. Significant discrepances are found in a number of cases, which can apparently be explained by insufficient accuracy of the estimated inclinations of the stars to the line of sight. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Astrophysical Bulletin Springer Journals

Magnetic configurations of the fast CP rotators HD3360, HD4778, HD5737, HD112413, and HD215441

Astrophysical Bulletin , Volume 64 (1) – Feb 22, 2009

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Publisher
Springer Journals
Copyright
Copyright © 2009 by Pleiades Publishing, Ltd.
Subject
Physics; Astronomy, Astrophysics and Cosmology
ISSN
1990-3413
eISSN
1990-3421
DOI
10.1134/S1990341309010040
Publisher site
See Article on Publisher Site

Abstract

The method of “magnetic charges” is used to model magnetic fields of five rapidly rotating stars (P < 25d) and to find the basic parameters of their magnetic fields. A table containing all the modeling results obtained using the adopted method as well as the parameters obtained for the same stars by other authors is presented. Significant discrepances are found in a number of cases, which can apparently be explained by insufficient accuracy of the estimated inclinations of the stars to the line of sight.

Journal

Astrophysical BulletinSpringer Journals

Published: Feb 22, 2009

References