An Accreting, Anomalously Low Mass Black Hole at the Center of Low Mass Galaxy IC 750
arXiv:2006.01114 · doi:10.3847/1538-4357/ab9944
Abstract
We present a multi-wavelength study of the active galactic nucleus in the nearby ( Mpc) low mass galaxy IC 750, which has circumnuclear 22 GHz water maser emission. The masers trace a nearly edge-on, warped disk 0.2 pc in diameter, coincident with the compact nuclear X-ray source which lies at the base of the kpc-scale extended X-ray emission. The position-velocity structure of the maser emission indicates the central black hole (BH) has a mass less than . Keplerian rotation curves fitted to these data yield enclosed masses between and , with a mode of . Fitting the optical spectrum, we measure a nuclear stellar velocity dispersion ~{\rm km~s} From near-infrared photometry, we fit a bulge mass of and a stellar mass of . The mass upper limit of the intermediate mass black hole in IC 750 falls roughly two orders of magnitude below the relation and roughly one order of magnitude below the and relations -- larger than the relations' intrinsic scatters of (0.58 0.09) dex, 0.69 dex, and (0.65 0.09) dex, respectively. These offsets could be due to larger scatter at the low mass end of these relations. Alternatively, black hole growth is intrinsically inefficient in galaxies with low bulge and/or stellar masses, which causes the black holes to be under-massive relative to their hosts, as predicted by some galaxy evolution simulations.
arXiv commentAccepted for publication in ApJ
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