Optical polarization from magnetized cataclysmic variables

Details Optical polarization from magnetized cataclysmic variables Optical polarization from magnetized cataclysmic variables

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.210p..15b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 210, Sept. 1, 1984, p. 15P-18P.

Astronomy and Astrophysics

Astronomy

9

Cataclysmic Variables, Magnetic Stars, Optical Polarization, Stellar Radiation, Binary Stars, White Dwarf Stars

Scientific paper

The absence of optically polarized radiation from certain cataclysmic
variables has been interpreted, by a number of authors, to imply that
the white dwarfs' magnetic field is weaker (less than about 10 to the
7th G) than in the AM Her binaries. Here, it is shown that this
interpretation is, in general, incorrect.

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