The intrinsic linear polarization of 53 Camelopardalis and alpha 2 Canum Venaticorum

Details The intrinsic linear polarization of 53 Camelopardalis and alpha 2 Canum Venaticorum The intrinsic linear polarization of 53 Camelopardalis and alpha 2 Canum Venaticorum

Jan 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mnras.166....1k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 166, Jan. 1974, p. 1-18.

Astronomy and Astrophysics

Astronomy

41

A Stars, Magnetic Stars, Polarization Characteristics, Stellar Spectra, Bandwidth, H Beta Line, Light Curve, Stellar Magnetic Fields, Tables (Data), Ultraviolet Spectra

Scientific paper

The intrinsic phase-dependent linear polarization of two magnetic Ap stars is studied. The polarization characteristics in a broad blue filter band and in the ultraviolet are outlined, and the mechanisms of polarization are examined. The blue band polarization of 53 Cam (corrected by removing the stellar component) is found to be compatible with an oblique rotator whose angular parameters are in essential agreement with those deduced by Landstreet (1970) and by Huchra (1972).

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