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Cited by 498

The DOI matches its Crossref record; 140 of the 140 references it cites were found in a registry or an index.

The Supermassive Black Hole at the Galactic Center

Open access
Melia, Fulvio, Falcke, Heino·2001·Annual Review of Astronomy and Astrophysics

Abstract

▪ Abstract The inner few parsecs at the Galactic Center have come under intense scrutiny in recent years, in part due to the exciting broad-band observations of this region, but also because of the growing interest from theorists motivated to study the physics of black hole accretion, magnetized gas dynamics, and unusual star formation. The Galactic Center is now known to contain arguably the most compelling supermassive black hole candidate, weighing in at a little over 2.6 million suns. Its interaction with the nearby environment, comprised of clusters of evolved and young stars, a molecular dusty ring, ionized gas streamers, diffuse hot gas, and a hypernova remnant, is providing a wealth of accretion phenomenology and high-energy processes for detailed modeling. In this review, we summarize the latest observational results and focus on the physical interpretation of the most intriguing object in this region—the compact radio source Sgr A*, thought to be the radiative manifestation of the supermassive black hole.

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Crossref · 10.1146/annurev.astro.39.1.309

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Metadata

Authors
Melia, F., & Falcke, H.
Venue
Annual Review of Astronomy and Astrophysics
Published
2001-09
Volume
39
Issue
1
Pages
309-352
ISSN
  • 0066-4146 (ISSN-L)
  • 1545-4282
OpenAlex
W2148783522
Cited by
498
References
140
FWCI
5.05
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The Supermassive Black Hole at the Galactic Center. https://app.cochat.ai/papers/10.1146/annurev.astro.39.1.309
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Melia, F., & Falcke, H. (2001). The Supermassive Black Hole at the Galactic Center. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.39.1.309

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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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