The origin of X-rays from dwarf novae in quiescence.

Details The origin of X-rays from dwarf novae in quiescence. The origin of X-rays from dwarf novae in quiescence.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..163m&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 163 - 164

Astronomy and Astrophysics

Astrophysics

3

Dwarf Novae: X Rays, White Dwarfs: Accretion Disks, White Dwarfs: Stellar Coronae

Scientific paper

The formation of a hot corona above the underlying cool accretion disk leads to an evaporation of the inner disk around the white dwarf. The mass flow via the corona is of order 10-11Msun/y. X-rays originate mainly from the dense thermal boundary layer around the white dwarf and partially from the lower corona above the disk. The authors determine the spectrum of the radiation.

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