Broad-band linear polarization and magnetic intensification in rotating magnetic stars

Details Broad-band linear polarization and magnetic intensification in rotating magnetic stars Broad-band linear polarization and magnetic intensification in rotating magnetic stars

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...249..228l&link_type=abstract

Astrophysical Journal, Part 1, vol. 249, Oct. 1, 1981, p. 228-237.

Computer Science

Numerical Analysis

28

Linear Polarization, Magnetic Stars, Stellar Magnetic Fields, Stellar Rotation, Variable Stars, Zeeman Effect, Magnetic Field Configurations, Numerical Analysis, Spectrum Analysis, Stellar Spectra

Scientific paper

Magnetic intensification is proposed as a mechanism to explain the general features of the variable broad-band linear polarization emerging from rotating magnetic stars. This mechanism is studied in detail, and some efforts are made to investigate the wide variety of polarization diagrams that can result from it. Theoretical results are compared with direct observations of the variable magnetic star 53 Cam to determine its geometric and magnetic configuration.

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