Disks and jets around a super-critically accreting black hole

Details Disks and jets around a super-critically accreting black hole Disks and jets around a super-critically accreting black hole

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1053..357o&link_type=abstract

OBSERVATIONAL EVIDENCE FOR BLACK HOLES IN THE UNIVERSE: Proceedings of the 2nd Kolkata Conference on Observational Evidence for

Computer Science

Infall, Accretion, And Accretion Disks, Galactic Nuclei, Circumnuclear Matter, And Bulges, Hydrodynamics

Scientific paper

Recent observations have revealed a number of the ultra-luminous X-ray Sources (ULXs) in nearby galaxies. A kind of the ULXs may originate from super-critically accreting stellar-mass black holes whose accretion rates exceed far the Eddington critical accretion rate. Several authors have developed theoretical models of the super-critical accretion disk, taking account of the effects of outflow and advection. Based on the theoretical models, we examine the super-critical accretion disk and outflows by 2D radiation hydrodynamical calculations, and compare the results with the SS 433 jets.

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