The system AM HER equals 4U 1814 plus 50

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Binary Stars, Magnetic Stars, Stellar Spectrophotometry, White Dwarf Stars, X Ray Sources, X Ray Spectra, Infrared Spectra, Linear Polarization, Orbital Elements, Periodic Variations, Radial Velocity, Stellar Mass Accretion, Stellar Models, Stellar Rotation, Tables (Data)

Scientific paper

The binary system AM Herculis equals 4U 1814 plus 50 gives the first well ascertained example of an X-ray emitting magnetic white dwarf. The orbital period (3.1h) is apparent from X-ray to IR frequencies and in linear and circular polarization. Since the time of the identification of the X-ray source the system has been extensively studied. The observations (which range from 1 MeV to 20 microns) are reviewed and compared with the present theory of X-ray emitting white dwarfs.

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