The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.
What drives the growth of black holes?
Open accessAbstract
Massive black holes (BHs) are at once exotic and yet ubiquitous, residing in the centers of massive galaxies in the local Universe. Recent years have seen remarkable advances in our understanding of how these BHs form and grow over cosmic time, during which they are revealed as active galactic nuclei (AGN). However, despite decades of research, we still lack a coherent picture of the physical drivers of BH growth, the connection between the growth of BHs and their host galaxies, the role of large-scale environment on the fueling of BHs, and the impact of BH-driven outflows on the growth of galaxies. In this paper we review our progress in addressing these key issues, motivated by the science presented at the “What Drives the Growth of Black Holes?” workshop held at Durham on 26 th ‐29 th July 2010, and discuss how these questions may be tackled with current and future facilities.
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Cites
THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., Prieto, C. A., An, D., Anderson, K. S. J., Anderson, S. F., Annis, J., Bahcall, N. A., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/182/2/543 · Cited by 5,341
On the Gravitational Stability of a Disk of Stars
Toomre, A. (1964) · The Astrophysical Journal · doi:10.1086/147861 · Cited by 3,349 · cited 2×
“For example, an isothermal gas disc is expected to become unstable when Σg > csκ πG , (3) which is equivalent to Q < 1 in terms of the Toomre parameter (e.g., Toomre, 1964; Thompson et al., 2005; McKee & Ostriker, 2007).”
BackgroundThe Two Young Star Disks in the Central Parsec of the Galaxy: Properties, Dynamics, and Formation
Paumard, T., Genzel, R., Martins, F., Nayakshin, S., Beloborodov, A. M., Levin, Y., Trippe, S., Eisenhauer, F., Ott, T., Gillessen, S., et al. (2006) · The Astrophysical Journal · doi:10.1086/503273 · Cited by 690
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Discovery of Variable Iron Fluorescence from Reflection Nebulae in the Galactic Center
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“These data suggest that Sgr A* may have been up-to ≈ 3 orders of magnitude brighter ≈ 100 years ago (e.g., Muno et al., 2007; Ponti et al., 2010).”
Background
Cited by
Buchner, J., Georgakakis, A., Nandra, K., Hsu, L., Rangel, C., Brightman, M., Merloni, A., Salvato, M., Donley, J., & Kocevski, D. (2014) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201322971 · Cited by 1,644
The eROSITA X-ray telescope on SRG
Predehl, P., Andritschke, R., Arefiev, V., Babyshkin, V., Batanov, O., Becker, W., Böhringer, H., Bogomolov, A., Boller, T., Borm, K., et al. (2021) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202039313 · Cited by 897
Active galactic nuclei: what’s in a name?
Padovani, P., Alexander, D. M., Assef, R. J., De Marco, B., Giommi, P., Hickox, R. C., Richards, G. T., Smolčić, V., Hatziminaoglou, E., Mainieri, V., et al. (2017) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-017-0102-9 · Cited by 666
Self-citationThe Illustris simulation: the evolving population of black holes across cosmic time
Sijacki, D., Vogelsberger, M., Genel, S., Springel, V., Torrey, P., Snyder, G. F., Nelson, D., & Hernquist, L. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1340 · Cited by 637
Simpson, J. M., Swinbank, A. M., Smail, I., Alexander, D. M., Brandt, W. N., Bertoldi, F., de Breuck, C., Chapman, S. C., Coppin, K. E. K., da Cunha, E., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/788/2/125 · Cited by 326
Self-citation
Metadata
- Authors
- Alexander, D. M., & Hickox, R. C.
- Venue
- New Astronomy Reviews
- Publisher
- Elsevier BV
- Published
- 2012-06
- Volume
- 56
- Issue
- 4
- Pages
- 93-121
- ISSN
- 1387-6473 (ISSN-L)
- OpenAlex
- W2167019439
- Cited by
- 568
- References
- 5
- FWCI
- 12.27
- Type
- journal article
- Language
- en
- Open access
- green
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