Two-pole emission in AM Herculis-type systems

Details Two-pole emission in AM Herculis-type systems Two-pole emission in AM Herculis-type systems

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236...31m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Jan. 1, 1989, p. 31-45.

Astronomy and Astrophysics

Astronomy

38

Magnetic Stars, Stellar Radiation, Variable Stars, White Dwarf Stars, Cyclotron Radiation, Linear Polarization

Scientific paper

Data for several AM Herculis-type variables are used to determine the field directions at the emission regions and the orbital inclinations. Self-consistent values are derived for AM Herculis, VV Puppis, and EF Eri. Additional assumptions produce a geometrical model that can explain observations of AM Herculis and VV Puppis. It is suggested that the field distribution of EF Eri may be a quadrupole.

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