The DOI matches its Crossref record; 41 of the 41 references it cites were found in a registry or an index.
MAJOR GALAXY MERGERS ONLY TRIGGER THE MOST LUMINOUS ACTIVE GALACTIC NUCLEI
Open accessAbstract
Using multiwavelength surveys of active galactic nuclei (AGNs) across a wide range of bolometric luminosities (10 43 < L bol (erg s −1 ) <5 × 10 46 ) and redshifts (0 < z < 3), we find a strong, redshift-independent correlation between the AGN luminosity and the fraction of host galaxies undergoing a major merger. That is, only the most luminous AGN phases are connected to major mergers, while less luminous AGNs appear to be driven by secular processes. Combining this trend with AGN luminosity functions to assess the overall cosmic growth of black holes, we find that ∼50% by mass is associated with major mergers, while only 10% of AGNs by number, the most luminous, are connected to these violent events. Our results suggest that to reach the highest AGN luminosities—where the most massive black holes accreted the bulk of their mass—a major merger appears to be required. The luminosity dependence of the fraction of AGNs triggered by major mergers can successfully explain why the observed scatter in the M –σ relation for elliptical galaxies is significantly lower than in spirals. The lack of a significant redshift dependence of the L bol – f merger relation suggests that downsizing, i.e., the general decline in AGN and star formation activity with decreasing redshift, is driven by a decline in the frequency of major mergers combined with a decrease in the availability of gas at lower redshifts.
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Cites
Energy input from quasars regulates the growth and activity of black holes and their host galaxies
Di Matteo, T., Springel, V., & Hernquist, L. (2005) · Nature · doi:10.1038/nature03335 · Cited by 3,353
Stellar masses and star formation histories for 105galaxies from the Sloan Digital Sky Survey
Kauffmann, G., Heckman, T. M., Simon White, D. M., Charlot, S., Tremonti, C., Brinchmann, J., Bruzual, G., Peng, E. W., Seibert, M., Bernardi, M., et al. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06291.x · Cited by 2,417
Ultraluminous infrared galaxies and the origin of quasars
Sanders, D. B., Soifer, B. T., Elias, J. H., Madore, B. F., Matthews, K., Neugebauer, G., & Scoville, N. Z. (1988) · The Astrophysical Journal · doi:10.1086/165983 · Cited by 2,072
Galaxy harassment and the evolution of clusters of galaxies
Moore, B., Katz, N., Lake, G., Dressler, A., & Oemler, A. (1996) · Nature · doi:10.1038/379613a0 · Cited by 1,740
Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
Kormendy, J., & Kennicutt, R. C. (2004) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.134024 · Cited by 1,732
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
A unified model for the evolution of galaxies and quasars
Kauffmann, G., & Haehnelt, M. (2000) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2000.03077.x · Cited by 1,179
SECULAR EVOLUTION AND THE FORMATION OF PSEUDOBULGES IN DISK GALAXIESPreprint
Kormendy, J., Kennicutt, R. C., & words, K. (2004) · Cited by 1,152
Ueda, Y., Akiyama, M., Ohta, K., & Miyaji, T. (2003) · The Astrophysical Journal · doi:10.1086/378940 · Cited by 1,105
Galaxy harassment and the evolution of clusters of galaxies
Moore, B., Katz, N., Lake, G., Dressler, A., & Oemler, A. E. (1995) · CERN Document Server (European Organization for Nuclear Research) · Cited by 969
Cited by
Silk, J. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/772/2/112 · Cited by 258
Using transfer learning to detect galaxy mergers
Ackermann, S., Schawinski, K., Zhang, C., Weigel, A. K., & Turp, M. D. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1398 · Cited by 137
Self-citationCosmological Simulations of Quasar Fueling to Subparsec Scales Using Lagrangian Hyper-refinement
Anglés-Alcázar, D., Quataert, E., Hopkins, P. F., Somerville, R. S., Hayward, C. C., Faucher-Giguère, C.-A., Bryan, G. L., Kereš, D., Hernquist, L., & Stone, J. M. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac09e8 · Cited by 118
What drives the growth of black holes: A decade of progress
Alexander, D. M., Hickox, R. C., Aird, J., Combes, F., Costa, T., Habouzit, M., Harrison, C. M., Leng, R. I., Morabito, L. K., Uckelman, S. L., et al. (2025) · New Astronomy Reviews · doi:10.1016/j.newar.2025.101733 · Cited by 18
Metadata
- Authors
- Treister, E., Schawinski, K., Urry, C. M., & Simmons, B. D.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2012-10-04
- Volume
- 758
- Issue
- 2
- Pages
- L39
- ISSN
- 2041-8205 (ISSN-L)
- 2041-8213
- OpenAlex
- W1991788629
- Cited by
- 385
- References
- 41
- FWCI
- 16.12
- Type
- journal article
- Language
- en
- Open access
- bronze
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