An accretion model for the growth of the central black hole associated with ionization instability in quasars

Details An accretion model for the growth of the central black hole associated with ionization instability in quasars An accretion model for the growth of the central black hole associated with ionization instability in quasars

2002-11-19

arxiv.org/abs/astro-ph/0211419v1

Astrophys.J. 590 (2003) 52-57

Astronomy and Astrophysics

Astrophysics

submitted to ApJ, 15 pages

Scientific paper

10.1086/375007

A possible accretion model associated with the ionization instability of
quasar disks is proposed to address the growth of the central black hole
harbored in the host galaxy.The mass ratio between black hole and its host
galactic bulge is a nature consequence of our model.

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