Inner edge of accretion disks in low mass X-ray binaries.

Details Inner edge of accretion disks in low mass X-ray binaries. Inner edge of accretion disks in low mass X-ray binaries.

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sccha..38.1117l&link_type=abstract

Science in China, Series A, Vol. 38, No. 9, p. 1117 - 1126

Physics

X-Ray Binaries: Accretion Disks, Accretion Disks: X-Ray Spectra, Accretion Disks: Oscillations

Scientific paper

The magnitude of the inner edge of accretion disks in low mass X-ray binaries is controversial in theoretical considerations and observations. Using the inner bondary conditions of accretion disks the inner disk radius has been calculated by taking into account the effect of feedback radiation and the deviation of disk rotation from Keplerian. Results have been applied to the observations and possible interpretations have been proposed for the X-ray spectra and quasiperiodic oscillations.

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