On subcritically accreting black holes

Details On subcritically accreting black holes On subcritically accreting black holes

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979nciml..26..239r&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 26, Oct. 20, 1979, p. 239-242.

Astronomy and Astrophysics

Astronomy

3

Astronomical Models, Black Holes (Astronomy), Stellar Mass Accretion, X Ray Sources, Emission Spectra, Interstellar Space, Neutron Stars, Stellar Luminosity

Scientific paper

A model is developed for isolated black holes accreting material from interstellar space at an accretion rate such that the X-ray luminosity is subcritical. It is assumed that the X-rays are produced in a disklike shell at a radius of the order of 10,000 times the black-hole mass, rather than near the hole's surface. Some predictions of this model are discussed for X-ray burst sources and the bizarre emission-line object SS433.

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