A Fundamental Relation Between Compact Stellar Nuclei, Supermassive Black Holes, and Their Host Galaxies

Details A Fundamental Relation Between Compact Stellar Nuclei, Supermassive Black Holes, and Their Host Galaxies A Fundamental Relation Between Compact Stellar Nuclei, Supermassive Black Holes, and Their Host Galaxies

2006-03-30

arxiv.org/abs/astro-ph/0603840v3

Astrophys.J.644:L21-L24,2006

Astronomy and Astrophysics

Astrophysics

ApJ Letters, Accepted. Postscript and PDF versions of the manuscript (with full resolution figures) can also be retreived from

Scientific paper

10.1086/505388

Imaging surveys with the Hubble Space Telescope (HST) have shown that roughly 50-80% of low- and intermediate-luminosity galaxies contain a compact stellar nucleus at their center, regardless of host galaxy morphological type. We combine HST imaging for early-type galaxies from the ACS Virgo Cluster Survey with ground-based long-slit spectra from KPNO to show that the masses of compact stellar nuclei in Virgo Cluster galaxies obey a tight correlation with the masses of the host galaxies. The same correlation is obeyed by the supermassive black holes (SBHs) found in predominantly massive galaxies. The compact stellar nuclei in the Local Group galaxies M33 and NGC205 are also found to fall along this same scaling relation. These results indicate that a generic by-product of galaxy formation is the creation of a Central Massive Object (CMO) -- either a SBH or a compact stellar nucleus -- that contains a mean fraction, ~ 0.2%, of the total galactic mass. In galaxies with masses greater than a few times 10^10 solar masses, SBHs appear to be the dominant mode of CMO formation.

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