EUVE Spectroscopy of the Accretion Region in AM Herculis

Details EUVE Spectroscopy of the Accretion Region in AM Herculis EUVE Spectroscopy of the Accretion Region in AM Herculis

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nasa.reptv....p&link_type=abstract

Technical Report, NASA/CR-97-206178; NAS 1.26:206178; CAL-2718 Columbia Astrophysics Lab.

Astronomy and Astrophysics

Astrophysics

White Dwarf Stars, Stellar Spectra, Cataclysmic Variables, Energy Conversion, Gravitational Binding Energy, Photosphere, Stellar Atmospheres, Fourier Transformation, Extreme Ultraviolet Explorer Satellite, Spectroscopic Analysis, Extreme Ultraviolet Radiation, X Rays, Accretion Disks, Emission Spectra, Line Spectra

Scientific paper

Progress in determining the gravitational energy conversion balance in
accreting white dwarf stars is reported. Detailed photospheric spectra
of the white dwarf stars in the brightest magnetic cataclysmic binaries,
in the region where most of the energy is radiated by the stellar
atmosphere - in the extreme ultraviolet band is obtained.

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