Supermassive black holes and central star clusters: Connection with the host galaxy kinematics and color

The relationship between the masses of the central, supermassive black holes (M (bh)) and of the nuclear star clusters (M (nc)) of disk galaxies with various parameters galaxies are considered: the rotational velocity at R = 2 kpc V ((2)), the maximum rotational velocity V (max), the indicative dynamical mass M (25), the integrated mass of the stellar populationM (*), and the integrated color index B-V. The rotational velocities andmasses of the central objects were taken from the literature. ThemassM (nc) correlatesmore closely with the kinematic parameters and the disk mass than M (bh), including with the velocity V (max), which is closely related to the virial mass of the dark halo. On average, lenticular galaxies are characterized by higher massesM (bh) compared to other types of galaxies with similar characteristics. The dependence of the blackhole mass on the color index is bimodal: galaxies of the red group (red-sequence) with B-V > 0.6-0.7 which are mostly early-type galaxies with weak star formation, differ appreciably from blue galaxies, which have higher values of M (nc) and M (bh). At the dependences we consider between the masses of the central objects and the parameters of the host galaxies (except for the dependence of M (bh) on the central velocity dispersion), the red-group galaxies have systematically higher M (bh) values, even when the host-galaxy parameters are similar. In contrast, in the case of nuclear star clusters, the blue and red galaxies form unified sequences. The results agree with scenarios in which most red-group galaxies form as a result of the partial or complete loss of interstellar gas in a stage of high nuclear activity in galaxies whose central black-hole masses exceed 10(6)-10(7) M (aS (TM)) (depending on the mass of the galaxy itself). The bulk of disk galaxies with M (bh) > 10(7) M (aS (TM)) are lenticular galaxies (types S0, E/S0) whose disks are practically devoid of gas.