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.
Astrophysical Bulletin – Springer Journals
Published: Feb 22, 2009