The DOI matches its Crossref record; 38 of the 38 references it cites were found in a registry or an index.
Axisymmetric Dynamical Models of the Central Regions of Galaxies
Open accessAbstract
We present axisymmetric, orbit superposition models for 12 galaxies using data taken with the Hubble Space Telescope ( HST ) and ground-based observatories. In each galaxy, we detect a central black hole (BH) and measure its mass to accuracies ranging from 10% to 70%. We demonstrate that in most cases the BH detection requires both the HST and ground-based data. Using the ground-based data alone does provide an unbiased measure of the BH mass (provided that they are fitted with fully general models), but at a greatly reduced significance. The most significant correlation with host galaxy properties is the relation between the BH mass and the velocity dispersion of the host galaxy; we find no other equally strong correlation and no second parameter that improves the quality of the mass-dispersion relation. We are also able to measure the stellar orbital properties from these general models. The most massive galaxies are strongly biased to tangential orbits near the BH, consistent with binary BH models, while lower mass galaxies have a range of anisotropies, consistent with an adiabatic growth of the BH.
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Cites
A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies
Ferrarese, L., & Merritt, D. (2000) · The Astrophysical Journal · doi:10.1086/312838 · Cited by 4,417
Spline Models for Observational Data
Wahba, G. (1990) · doi:10.1137/1.9781611970128 · Cited by 4,184
Bayesian-Based Iterative Method of Image Restoration*
Richardson, W. H. (1972) · Journal of the Optical Society of America · doi:10.1364/josa.62.000055 · Cited by 4,160
The Demography of Massive Dark Objects in Galaxy Centers
Magorrian, J., Tremaine, S., Richstone, D., Bender, R., Bower, G., Dressler, A., Faber, S. M., Gebhardt, K., Green, R., Grillmair, C., et al. (1998) · The Astronomical Journal · doi:10.1086/300353 · Cited by 4,007
Self-citationAn iterative technique for the rectification of observed distributions
Lucy, L. B. (1974) · The Astronomical Journal · doi:10.1086/111605 · Cited by 3,866 · cited 1×
“After the subexposures were compared to detect and eliminate cosmic-ray events, they were combined and then deconvolved using Lucy (1974) and Richardson (1972) deconvolution.”
MethodA 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
Self-citationThe Slope of the Black Hole Mass versus Velocity Dispersion Correlation
Tremaine, S., Gebhardt, K., Bender, R., Bower, G., Dressler, A., Faber, S. M., Filippenko, A. V., Green, R., Grillmair, C., Ho, L. C., et al. (2002) · The Astrophysical Journal · doi:10.1086/341002 · Cited by 2,617
Self-citationInward Bound—The Search for Supermassive Black Holes in Galactic Nuclei
Kormendy, J., & Richstone, D. (1995) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.33.090195.003053 · Cited by 2,544
Self-citationComprehensive stellar population models and the disentanglement of age and metallicity effects
Worthey, G. (1994) · The Astrophysical Journal Supplement Series · doi:10.1086/192096 · Cited by 1,699
Third Reference Catalogue of Bright Galaxies: Volume II
de Vaucouleurs, G., de Vaucouleurs, A., Corwin, H. G., Buta, R. J., Paturel, G., & Fouqué, P. (1991) · Springer eBooks · doi:10.1007/978-1-4757-4360-9 · Cited by 1,327
Cited by
On the Black Hole Mass-Bulge Mass Relation
Hring, N., & Rix, H.-W. (2004) · The Astrophysical Journal · doi:10.1086/383567 · Cited by 1,626
THE M-σ AND M-L RELATIONS IN GALACTIC BULGES, AND DETERMINATIONS OF THEIR INTRINSIC SCATTER
Gültekin, K., Richstone, D. O., Gebhardt, K., Lauer, T. R., Tremaine, S., Aller, M. C., Bender, R., Dressler, A., Faber, S. M., Filippenko, A. V., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/698/1/198 · Cited by 1,533
Self-citationSupermassive Black Holes in Galactic Nuclei: Past, Present and Future Research
Ferrarese, L., & Ford, H. (2005) · Space Science Reviews · doi:10.1007/s11214-005-3947-6 · Cited by 850
Structure and Formation of Elliptical and Spheroidal Galaxies
Bender, R. (2016) · doi:10.15781/t28g8fm0v · Cited by 555
Self-citationStructure and Kinematics of Early-Type Galaxies from Integral Field Spectroscopy
Cappellari, M. (2016) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082214-122432 · Cited by 507
Metadata
- Authors
- Gebhardt, K., Richstone, D., Tremaine, S., Lauer, T. R., Bender, R., Bower, G., Dressler, A., Faber, S. M., Filippenko, A. V., Green, R., Grillmair, C., Ho, L. C., Kormendy, J., Magorrian, J., & Pinkney, J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2003-01-20
- Volume
- 583
- Issue
- 1
- Pages
- 92-115
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2133907243
- Cited by
- 393
- References
- 38
- FWCI
- 17.98
- Type
- journal article
- Language
- en
- Open access
- bronze
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