Luminosity Limit of Super-Eddington Accretion onto Black Holes
-
Abstract
The luminosity limit is derived for the Super-Eddington accretion by obtaining the self-similar solution. The maximum luminosity is about 4.0 x 1037 erg/s(M/Mסּ) or so (significantly less than the Eddington luminosity) due to photon trapping although the accretion rate is Super-Eddington. The radiation spectrum is found to be universal as Fν ∝ ν-1.
Article Text
-
-
-
About This Article
Cite this article:
WANG Jian-min. Luminosity Limit of Super-Eddington Accretion onto Black Holes[J]. Chin. Phys. Lett., 1999, 16(6): 467-468.
WANG Jian-min. Luminosity Limit of Super-Eddington Accretion onto Black Holes[J]. Chin. Phys. Lett., 1999, 16(6): 467-468.
|
WANG Jian-min. Luminosity Limit of Super-Eddington Accretion onto Black Holes[J]. Chin. Phys. Lett., 1999, 16(6): 467-468.
WANG Jian-min. Luminosity Limit of Super-Eddington Accretion onto Black Holes[J]. Chin. Phys. Lett., 1999, 16(6): 467-468.
|