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29 March 2024
 
  » arxiv » astro-ph/0211419

 Article overview


An accretion model for the growth of the central black hole associated with ionization instability in quasars
Y. Lu ; K.S. Cheng ; S.N. Zhang ;
Date 19 Nov 2002
Journal Astrophys.J. 590 (2003) 52-57
Subject astro-ph
AffiliationNational Astronomical Observatories, Chinese Academy of Sciences, Beijing, China), K.S. Cheng (Department of Physics, The University of Hong Kong, Hong Kong, China), S.N. Zhang (Physics Department and Center for Astrophysics, Tsinghua University, Beiji
AbstractA 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.
Source arXiv, astro-ph/0211419
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