Formation of quasar nuclei in the hearts of ultraluminous infrared galaxies

We investigate whether or not supermassive black holes (SMBHs) with mass gr eater than or similar to 10(8) M-. can be made in the hearts of ultralumino us infrared galaxies (ULIGs) during the course of mergers between/among gas -rich galaxies. (1) If one progenitor galaxy had a seed SMBH with mass of s imilar to 10(7) M-., this seed SMBH can grow up to greater than or similar to 10(8) M, due to efficient Bondi-type gas accretion during the course of merger, given a gas density in the circumnuclear region of n(H) similar to 10(3) cm(-3). (2) Even if there was no progenitor galaxy with a seed SMBH, star clusters with compact remnants (neutron stars and/or black holes) prod uced in the circumnuclear starbursts can merge into the merger center withi n a dynamical timescale of similar to 10(9) yr to form an SMBH with greater than or similar to 10(8) M-.. Note, however, that the contribution of comp act remnants supplied from hidden star clusters is necessary to lead to the formation of an SMBH. In conclusion, the ULIGs observed in the local unive rse can make SMBHs in their centers during the course of merging either by gas accretion onto a seed SMBH or by dynamical relaxation of compact remnan ts made in the violent circumnuclear starbursts. Therefore, it is quite lik ely that the ULIGs will finally evolve to optically luminous quasars, as su ggested by Sanders et al.