A theory of the instability of disk accretion on to black holes and the variability of binary X-ray sources, galactic nuclei and quasars

Details A theory of the instability of disk accretion on to black holes and the variability of binary X-ray sources, galactic nuclei and quasars A theory of the instability of disk accretion on to black holes and the variability of binary X-ray sources, galactic nuclei and quasars

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.175..613s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 175, June 1976, p. 613-632. Translation.

Astronomy and Astrophysics

Astronomy

402

Binary Stars, Black Holes (Astronomy), Galactic Nuclei, Quasars, Thermal Instability, X Ray Sources, Asymptotic Methods, Disks (Shapes), Perturbation Theory, Standing Waves, Traveling Waves

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976MNRAS.175..613S

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