Sagittarius A and Its Environment
Abstract
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Integrity signals
Registry
Cites
Statistics
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The CND has a total mass of 10^5-6 M⊙ and hosts several clumps with densities of ~10^6-8 cm^-3 and gas temperatures of ~50 K.
“The CND has a total mass of 10 5 -6 M ⊙ and hosts several clumps with densities of ∼ 10 6 -8 cm -3 and gas temperatures of ∼ 50 K (Becklin et al. 1982; Brown & Liszt 1984; Genzel et al. 1985; Serabyn et al. 1986; Genzel et al. 2010; Hsieh et al. 2021).”
From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Brown & Liszt 1984
Cites
Positron-electron pairs in astrophysics
Burns, M. L., Harding, A. K., & Ramaty, R. (1983) · Cited by 255 · see citing works
The Large-Scale Characteristics of the Galaxy
(1979) · Springer eBooks · doi:10.1007/978-94-009-9503-1 · Cited by 240 · see citing works
Radio astronomy and the galactic system
van Woerden, H. C., & Pikel'Ner, S. B. (1969) · Academic Press eBooks · Cited by 156 · see citing works
Flagged first, then by citations
Cited by
Sorted by citations
THE GALACTIC CENTER ENVIRONMENT
Morris, M., & Serabyn, E. (1996) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.34.1.645 · Cited by 930 · see citing works
The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way
Sarkar, K. C. (2024) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-024-00152-1 · Cited by 34 · see citing works
“The CND has a total mass of 10 5 − 6 M ⊙ and hosts several clumps with densities of ∼ 10 6 − 8 cm − 3 and gas temperatures of ∼ 50 K (Becklin et al. 1982; Brown & Liszt 1984; Genzel et al. 1985; Serabyn et al. 1986; Genzel et al. 2010; Hsieh et al. 2021).”
Background
- Authors
- Brown, R. L., & Liszt, H. S.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 1984-09
- Volume
- 22
- Issue
- 1
- Pages
- 223-265
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2118812235
- Cited by
- 70
- References
- 3
- Citations by year
- 2026: 1 · 2025: 1 · 2024: 1 · 2016: 1 · 2014: 1 · 2012: 2
- FWCI
- 6.47
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Annual Review of Astronomy and Astrophysics (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- Sgr A*, Galactic Center, supermassive black holes, black hole environment, star clusters, X-ray sources
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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