Emission of X-ray and ultraviolet radiation during accretion of matter to nonmagnetic white dwarfs

Details Emission of X-ray and ultraviolet radiation during accretion of matter to nonmagnetic white dwarfs Emission of X-ray and ultraviolet radiation during accretion of matter to nonmagnetic white dwarfs

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980poast..28...47s&link_type=abstract

Postepy Astronomii, vol. 28, Jan.-Mar. 1980, p. 47-60. In Polish.

Astronomy and Astrophysics

Astronomy

Stellar Mass Accretion, Ultraviolet Astronomy, White Dwarf Stars, X Ray Astronomy, X Ray Stars, Absorption Spectra, Astronomical Models, Emission Spectra

Scientific paper

In the present paper, a mathematical model of radiation from an
accreting nonmagnetic white dwarf is constructed under the assumption
that the process is spherically symmetric and the star does not rotate.
The parameters characterizing the accretion to white dwarf are examined,
and possible mechanisms of X-ray and UV emission are proposed.

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