The DOI matches its Crossref record; 48 of the 48 references it cites were found in a registry or an index.
A Fundamental Relation between Compact Stellar Nuclei, Supermassive Black Holes, and Their Host Galaxies
Open accessAbstract
Imaging surveys with the Hubble Space Telescope ( HST ) have shown that ≈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 NGC 205 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 an SBH or a compact stellar nucleus—that contains a mean fraction, ≈0.2%, of the total galactic mass. In galaxies with masses greater than gal ~ a few × 10 10 ☉ , SBHs appear to be the dominant mode of CMO formation.
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Cites
Stellar population synthesis at the resolution of 2003
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Galactic Stellar and Substellar Initial Mass Function
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A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies
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Self-citationA Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion
Gebhardt, K., Bender, R., Bower, G., Dressler, A., Faber, S. M., Filippenko, A. V., Green, R., Grillmair, C., Ho, L. C., Kormendy, J., et al. (2000) · The Astrophysical Journal · doi:10.1086/312840 · Cited by 3,671
The Slope of the Black Hole Mass versus Velocity Dispersion Correlation
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The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
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Cited by
Formation of supermassive black holes
Volonteri, M. (2010) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-010-0029-x · Cited by 783
Mei, S., Blakeslee, J. P., Cote, P., Tonry, J. L., West, M. J., Ferrarese, L., Jordan, A., Peng, E. W., Anthony, A., & Merritt, D. (2007) · The Astrophysical Journal · doi:10.1086/509598 · Cited by 722
Self-citationStructure and Formation of Elliptical and Spheroidal Galaxies
Bender, R. (2016) · doi:10.15781/t28g8fm0v · Cited by 555
How do massive black holes get their gas?
Hopkins, P. F., & Quataert, E. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17064.x · Cited by 503
An expanded Mbh-σ diagram, and a new calibration of active galactic nuclei masses: The Mbh-σ diagram
Graham, A. W., Onken, C. A., Athanassoula, E., & Combes, F. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.18045.x · Cited by 422
Metadata
- Authors
- Ferrarese, L., Côté, P., Dalla Bontà, E., Peng, E. W., Merritt, D., Jordán, A., Blakeslee, J. P., Haşegan, M., Mei, S., Piatek, S., Tonry, J. L., & West, M. J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2006-05-19
- Volume
- 644
- Issue
- 1
- Pages
- L21-L24
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2057422331
- Cited by
- 368
- References
- 48
- FWCI
- 23.72
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Ferrarese, L., Côté, P., Dalla Bontà, E., Peng, E. W., Merritt, D., Jordán, A., Blakeslee, J. P., Haşegan, M., Mei, S., Piatek, S., Tonry, J. L., & West, M. J. (2006). A Fundamental Relation between Compact Stellar Nuclei, Supermassive Black Holes, and Their Host Galaxies. The Astrophysical Journal. https://doi.org/10.1086/505388
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