The DOI matches its Crossref record; 224 of the 224 references it cites were found in a registry or an index.
The Circumgalactic Medium
Open accessAbstract
The gas surrounding galaxies outside their disks or interstellar medium and inside their virial radii is known as the circumgalactic medium (CGM). In recent years this component of galaxies has assumed an important role in our understanding of galaxy evolution owing to rapid advances in observational access to this diffuse, nearly invisible material. Observations and simulations of this component of galaxies suggest that it is a multiphase medium characterized by rich dynamics and complex ionization states. The CGM is a source for a galaxy's star-forming fuel, the venue for galactic feedback and recycling, and perhaps the key regulator of the galactic gas supply. We review our evolving knowledge of the CGM with emphasis on its mass, dynamical state, and coevolution with galaxies. Observations from all redshifts and from across the electromagnetic spectrum indicate that CGM gas has a key role in galaxy evolution. We summarize the state of this field and pose unanswered questions for future research.
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“Observationally, the total mass and density profile of the CGM in MW-mass galaxies are poorly determined and this is likely to remain so for years to come”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Tumlinson et al. 2017
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Cited by
Sorted by citations
The milky way total mass profile as inferred from Gaia DR2
Cautun, M., Benítez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1017 · Cited by 332
“Observationally, the total mass and density profile of the CGM in MW-mass galaxies are poorly determined and this is likely to remain so for years to come (e.g. Tumlinson et al. 2017).”
BackgroundThe Milky Way total mass profile as inferred from Gaia DR2
Cautun, M., Benitez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2019) · arXiv · doi:10.48550/arxiv.1911.04557 · Cited by 335
Detection of large-scale X-ray bubbles in the Milky Way halo
Predehl, P., Sunyaev, R. A., Becker, W., Brunner, H., Burenin, R., Bykov, A., Cherepashchuk, A., Chugai, N., Churazov, E., Doroshenko, V., et al. (2020) · Nature · doi:10.1038/s41586-020-2979-0 · Cited by 234
Davies, J. J., Crain, R. A., Oppenheimer, B. D., & Schaye, J. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3201 · Cited by 167
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Metadata
- Authors
- Tumlinson, J., Peeples, M. S., & Werk, J. K.
- Affiliations
- Space Telescope Science Institute (US)
- University of Washington (US)
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2017-08-18
- Volume
- 55
- Issue
- 1
- Pages
- 389-432
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2561281082
- Cited by
- 1,147
- References
- 224
- Citations by year
- 2026: 122 · 2025: 181 · 2024: 173 · 2023: 154 · 2022: 114 · 2021: 134 · 2020: 106 · 2019: 101 · 2018: 57 · 2017: 5
- FWCI
- 7.43
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Annual Review of Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Keywords
- circumgalactic medium, galaxy evolution, multiphase gas, ionization state, galactic feedback, gas recycling, intergalactic medium
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