Titlebook: Upper Main Sequence Stars with Anomalous Abundances; Proceedings of the 9 C. R. Cowley,M. M. Dworetsky,C. Mégessier Conference proceedings

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Upper Main Sequence Stars with Anomalous Abundances978-94-009-4714-6Series ISSN 0067-0057 Series E-ISSN 2214-7985

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On the Spottedness, Magnetism and Internal Structure of StarsIt is hypothesized that kinematical structures within stellar interiors that are results of a self-organization of these interiors as thermodynamically open non-linear systems constitute the physical basis for stellar magnetism.

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Influence of the Magnetic Field on the Polarization of Radiation Scattered by Electrons in Stellar AThe radiation scattering by electrons play an important role for stars with the surface temperature ≥ 2.10. °K. Many among these stars have magnetic fields of the order 1 – 100 G. We shall consider the role of the field for the radiative transfer in continuum spectra.

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