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The nucleus of our Galaxy
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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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Polarization of the Thermal Emission from the Dust Ring at the Center of the Galaxy
Hildebrand, R. H., Davidson, J. A., Dotson, J. L., Figer, D. F., Novak, G., Platt, S. R., & Tao, L. (1993) · The Astrophysical Journal · doi:10.1086/173336 · Cited by 48
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Glass, I. S., Moneti, A., & Moorwood, A. F. M. (1990) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/242.1.55p · Cited by 47
Flux Density of Sagittarius A at lambda = 3 Millimeters
Wright, M. C. H., & Backer, D. C. (1993) · The Astrophysical Journal · doi:10.1086/173335 · Cited by 46
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Shocked molecular hydrogen emission from the centre of the Galaxy
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Self-citationSub-millimeter continuum emission from the Galactic center region
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On the origin of variable 511 keV line emission from the Galactic center region
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X-Ray Sources Near the Galactic Center Observed by UHURU
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Apparent proper motions of the galactic center compact radio source and PSR 1929+10
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Airborne far-infrared observations of the galactic center region
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A filamentary radio source near the Galactic Centre
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X-ray telescopes ART-P and ART-S for the granat project
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OH/IR stars within 50 parsecs of the Galactic center
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Self-citationAn electrodynamic model of the Galactic center
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A shocked-jet model of the Galactic center bridge and the radio arc
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Giant and supergiant stars with degenerate neutron cores
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High-resolution infrared mapping of the Galactic center - Imaging and lunar occultations
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Stellar encounters in the Galactic center - Formation of massive stars and close binaries
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Fine-scale structure in the -185 kilometers per second absorption by HCO(+) in the Galactic center
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On the Use of Field Intensity Measurements for the Determination of Broadcast Station Coverage
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Ionization state in and reddening to the center of the Galaxy
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THE DISTRIBUTION AND KINEMATICS OF THE IONIZED-GAS IN THE GALACTIC-CENTER REGION
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Self-citation
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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