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

Beijing; Center for Astrophysics; China); Chinese Academy of Sciences; Hong Kong; K.S. Cheng (Department of Physics; S.N. Zhang (Physics Department; The University of Hong Kong; Tsinghua University; Y. Lu (National Astronomical Observatories

arxiv: astro-ph/0211419 · v1 · submitted 2002-11-19 · 🌌 astro-ph

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

Y. Lu (National Astronomical Observatories , Chinese Academy of Sciences , Beijing , China) , K.S. Cheng (Department of Physics , The University of Hong Kong , Hong Kong , S.N. Zhang (Physics Department

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Center for Astrophysics Tsinghua University

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keywords blackholemodelaccretionassociatedcentralgrowthhost

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

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