Advection-Dominated Accretion Flows in Quiescent Dwarf Novae

Details Advection-Dominated Accretion Flows in Quiescent Dwarf Novae Advection-Dominated Accretion Flows in Quiescent Dwarf Novae

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.4105m&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #41.05; Bulletin of the American Astronomical Society, Vol. 32, p.1254

Astronomy and Astrophysics

Astronomy

Scientific paper

White dwarfs in quiescent dwarf novae could accrete via an Advection-Dominated Accretion Flow (ADAF), responsible for the X-ray Bremsstrahlung emission observed at temperatures ranging from a few keV to a few tens of keV. Spectral models for the continuum and line emission of an ADAF around a white dwarf are presented and the possibility of testing, with current instruments, the property of energy advection via the detection of X-ray lines formed in a flow with a sub-Keplerian rotation rate is emphasized.

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