The DOI matches its Crossref record; 214 of the 214 references it cites were found in a registry or an index.
The nucleus of our Galaxy
Open accessAbstract
The subject of this review is the central 100 parsecs of our Galaxy, with a strong focus on the central few parsecs. Observations of the electromagnetic spectrum over 13 orders of magnitude in wavelength show a broad range of phenomena involving a number of physical processes. We discuss the stellar and interstellar components, the importance of magnetic and gravitational forces, the evidence for stellar formation and a central massive black hole, and the origin and nature of ionization, outflows and interstellar gas dynamics.
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“Within the ionized cavity, different streams spiral in toward Sgr A ∗ with the closest approach at ∼ 0 . 04 pc where the mass inflow rate is estimated to be ∼ 10 -3 M ⊙ yr -1 (Genzel et al. 1994).”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Genzel et al. 1994
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Cites
Black Holes, White Dwarfs, and Neutron Stars
Shapiro, S. L., & Teukolsky, S. A. (1983) · Wiley eBooks · doi:10.1002/9783527617661 · Cited by 4,833
Tidal disruption of stars by black holes of 106–108 solar masses in nearby galaxies
Rees, M. J. (1988) · Nature · doi:10.1038/333523a0 · Cited by 1,673
Black Holes in Binary Systems: Observational Appearances
Shakura, N. I., & Sunyaev, R. (1973) · Springer eBooks · doi:10.1007/978-94-010-2585-0_13 · Cited by 1,506
Black Hole Models for Active Galactic Nuclei
Rees, M. J. (1984) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.22.090184.002351 · Cited by 1,484
Asymptotic Giant Branch Evolution and Beyond
Iben, I., & Renzini, A. (1983) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.21.090183.001415 · Cited by 1,265
Astronomical Measurements in the Infrared
Johnson, H. L. (1966) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.04.090166.001205 · Cited by 918
Hollenbach, D. J., & McKee, C. F. (1989) · The Astrophysical Journal · doi:10.1086/167595 · Cited by 850
Self-citationSome Physical parameters of early-type stars
Panagia, N. (1973) · The Astronomical Journal · doi:10.1086/111498 · Cited by 778
Star distribution around a massive black hole in a globular cluster
Bahcall, J. N., & Wolf, R. (1976) · The Astrophysical Journal · doi:10.1086/154711 · Cited by 755
A composite CO survey of the entire Milky Way
Dame, T. M., Ungerechts, H., Cohen, R. S., Geus, E. J. D., Grenier, I. A., May, J., Murphy, D. C., Nyman, L. Å., & Thaddeus, P. (1987) · The Astrophysical Journal · doi:10.1086/165766 · Cited by 672
Research works printed but not linked: 56
- Allen D A, 1990, MNRAS, 244, 706
- Altenhoff W J, 1978, Astron. Astrophys. Suppl., 35, 23
- Backer D C, 1994, Nature
- Blitz L, 1985, Astrophys. J., 143, 267
- Bouchet L, 1991, et al., 383, L45
- Catchpole R M, 1990, MNRAS, 247, 479
- Close L M, 1992, BAAS, 24, 1178
- Cohn H, 1980, Astrophys. J., 150, 163
- Cotera A S, 1992, BAAS, 24, 1262
- Diehl R, 1993, Astron. Astrophys. Suppl., 97, 181
- Downes D, 1978, Astron. Astrophys. Suppl., 35, 1
- Eckart A, 1991, The ESO Messenger, 65, 1
- Ekers R D, 1971, Astrophys. Lett., 9, 189
- Ekers R D, 1983, Astron. Astrophys., 122, 143
- Erickson E F, 1992, BAAS, 24, 1131
- Falcke H, 1993, Astron. Astrophys., 270, 102
- Gurzadyan V G, 1980, Astron. Astrophys., 86, 315
- Gwinn C R, 1991, 381, L43
- Haller J W, 1992, BAAS, 24, 1178
- Kormendy J, 1993, Ann. Rev. Astron. Astrophys.
- Krichbaum T, 1994, Astron. Astrophys.
- Lauer T R, 1994, Astrophys. J.
- Lesch P, 1993, Astron. Astrophys.
- Lindqvist M, 1992, Astron. Astrophys. Suppl., 92, 43
- Lindqvist M, 1992, Astron. Astrophys., 259, 118
- Liszt H S, 1983, Astron. Astrophys., 126, 341
- Lutz D, 1993, Astrophys. J., Z18, 214
- Maeder A, 1987, Astron. Astrophys., 182, 243
- Maeder A, 1988, Astron. Astrophys. (Suppl.), 76, 411
- Markevitch M, 1993, Nature
- Mezger P G, 1989, Astron. Astrophys., 209, 337
- Mezger P G, 1990, Astron. Astrophys., 228, 95
- Mirabel I F, 1991, Astron. Astrophys., 251, L43
- Moneti A, 1991, Memm. Soc. Astr. It. 62, 4, 755
- Najarro F, 1993, Astron. Astrophys.
- Oort J H, 1975, Astron. Astrophys., 41, 71
- Pauls T A, 1980, Astron. Astrophys., 85, 26
- Rees M J, Ann. Rev. Astron. Astrophys., 31
- 10.1086/185199 · DOI
- Rosa M R, 1992, Astron. Astrophys., 257, 515
- Schwarz U J, 1989, Astron. Astrophys., 215, 33
- Serabyn E, 1986, Astron. Astrophys., 169, 85
- Serabyn E, 1987, Astron. Astrophys., 184, 133
- Serabyn E, 1991, Astron. Astrophys., 242, 376
- Shakura N I, 1973, Astron. Astrophys., 24, 337
- Shibata K, 1987, Pub. Astr. Aoc. Jap., 39, 559
- Shields J, 1993, Astrophys. J.
- Skinner G K, Astron. Astrophys. Suppl., 97, 149
- Sunyaev R, et al Astron. Astrophys., 247, L29
- Tamura M, 1993, Astrophys. J.
- Tsuboi M, 1986, Astrophys. J., 92, 819
- von Linden S, 1993, Astron. Astrophys., 246, 146
- Werner M W, 1992, BAAS, 24, 1260
- 10.1086/168966 · DOI
- Zylka R, 1990, Astron. Astrophys., 234, 133
- Zylka R, 1992, Astron. Astrophys., 261, 119
Cited by
Sorted by citations
Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
Kormendy, J., & Ho, L. C. (2013) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082708-101811 · Cited by 4,421
Veilleux, S., Cecil, G. N., & Bland‐Hawthorn, J. (2005) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.43.072103.150610 · Cited by 1,464
Coevolution (Or Not) of Supermassive Black Holes and Host GalaxiesPreprint
Kormendy, J., & Ho, L. C. (2013) · Cited by 1,881
The Galactic Center massive black hole and nuclear star cluster
Genzel, R., Eisenhauer, F., & Gillessen, S. (2010) · Reviews of Modern Physics · doi:10.1103/revmodphys.82.3121 · Cited by 1,236
Self-citationWhat Powers Ultraluminous IRAS Galaxies?
Genzel, R., Lutz, D., Sturm, E., Egami, E., Kunze, D., Moorwood, A., Rigopoulou, D., Spoon, H., Sternberg, A., Tacconi-Garman, L., et al. (1997) · The Astrophysical Journal · doi:10.1086/305576 · Cited by 960
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Metadata
- Authors
- Genzel, R., Hollenbach, D., & Townes, C. H.
- Affiliations
- Max Planck Institute for Extraterrestrial Physics (DE)
- Venue
- Reports on Progress in Physics
- Publisher
- IOP Publishing
- Published
- 1994-05-01
- Volume
- 57
- Issue
- 5
- Pages
- 417-479
- ISSN
- 0034-4885 (ISSN-L)
- 1361-6633
- OpenAlex
- W2104012283
- Cited by
- 200
- References
- 214
- Citations by year
- 2026: 5 · 2025: 3 · 2024: 6 · 2023: 4 · 2022: 4 · 2021: 4 · 2020: 1 · 2019: 1 · 2018: 2 · 2017: 3 · 2016: 5 · 2015: 4 · 2014: 3 · 2013: 4 · 2012: 2
- FWCI
- 22.09
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Reports on Progress in Physics (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- galactic nuclei, Milky Way center, central parsec, stellar populations, interstellar medium, magnetic field, gravitational force, star formation, supermassive black holes, ionization, galactic outflows, interstellar gas dynamics
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