The DOI matches its Crossref record; 11 of the 11 references it cites were found in a registry or an index.
Active galactic nuclei as scaled-up Galactic black holes
Open accessAbstract
A long-standing question is whether active galactic nuclei (AGN) vary like Galactic black hole systems when appropriately scaled up by mass. If so, we can then determine how AGN should behave on cosmological timescales by studying the brighter and much faster varying Galactic systems. As X-ray emission is produced very close to the black holes, it provides one of the best diagnostics of their behaviour. A characteristic timescale—which potentially could tell us about the mass of the black hole—is found in the X-ray variations from both AGN and Galactic black holes, but whether it is physically meaningful to compare the two has been questioned. Here we report that, after correcting for variations in the accretion rate, the timescales can be physically linked, revealing that the accretion process is exactly the same for small and large black holes. Strong support for this linkage comes, perhaps surprisingly, from the permitted optical emission lines in AGN whose widths (in both broad-line AGN and narrow-emission-line Seyfert 1 galaxies) correlate strongly with the characteristic X-ray timescale, exactly as expected from the AGN black hole masses and accretion rates. So AGN really are just scaled-up Galactic black holes.
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Cites
Peterson, B. M., Ferrarese, L., Gilbert, K. M., Kaspi, S., Malkan, M. A., Maoz, D., Merritt, D., Netzer, H., Onken, C. A., Pogge, R. W., et al. (2004) · The Astrophysical Journal · doi:10.1086/423269 · Cited by 1,802
Lewin, W. H. G., & van der Klis, M. (2010) · CERN Document Server (European Organization for Nuclear Research) · Cited by 1,799
A Fundamental Plane of black hole activity
Merloni, A., Heinz, S., & Di Matteo, T. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-2966.2003.07017.x · Cited by 1,215
Falcke, H., Körding, E., & Markoff, S. (2004) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20031683 · Cited by 768
McClintock, J. E., & Remillard, R. A. (2006) · Cambridge University Press eBooks · doi:10.1017/cbo9780511536281.005 · Cited by 707
Measuring the broad-band power spectra of active galactic nuclei with RXTE
Uttley, P., McHardy, I. M., & Papadakis, I. E. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2002.05298.x · Cited by 456
Self-citationFalcke, H. D., Körding, E. G., & Markoff, S. (2003) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/0305335 · Cited by 441
Bentz, M. C., Peterson, B. M., Pogge, R. W., Vestergaard, M., & Onken, C. A. (2006) · The Astrophysical Journal · doi:10.1086/503537 · Cited by 403
Liu, B. F., Yuan, W., Meyer, F., Meyer‐Hofmeister, E., & Xie, G. Z. (1999) · The Astrophysical Journal · doi:10.1086/312383 · Cited by 129
D’Agostini, G. (2005) · arXiv (Cornell University) · doi:10.48550/arxiv.physics/0511182 · Cited by 82
Cited by
Vasudevan, R. V., & Fabian, A. C. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12328.x · Cited by 473
X-ray reverberation around accreting black holes
Uttley, P., Cackett, E. M., Fabian, A. C., Kara, E., & Wilkins, D. R. (2014) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-014-0072-0 · Cited by 466
Self-citationUltraluminous X-ray sources in the Chandra and XMM-Newton era
Feng, H., & Soria, R. (2011) · New Astronomy Reviews · doi:10.1016/j.newar.2011.08.002 · Cited by 323
Sánchez-Sáez, P., Lira, H., Martí, L., Sánchez-Pi, N., Arredondo, J., Bauer, F. E., Bayo, A., Cabrera-Vives, G., Donoso-Oliva, C., Estévez, P. A., et al. (2021) · The Astronomical Journal · doi:10.3847/1538-3881/ac1426 · Cited by 47
Metadata
- Authors
- McHardy, I. M., Koerding, E., Knigge, C., Uttley, P., & Fender, R. P.
- Venue
- Nature
- Published
- 2006-12
- Volume
- 444
- Issue
- 7120
- Pages
- 730-732
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W1985523694
- Cited by
- 676
- References
- 11
- FWCI
- 19.09
- Type
- journal article
- Language
- en
- Open access
- green
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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