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Cited by 443

The DOI matches its Crossref record; 165 of the 165 references it cites were found in a registry or an index.

INTERMEDIATE-MASS BLACK HOLES

Open access
COLEMAN MILLER, M., COLBERT, E. J. M.·2004·International Journal of Modern Physics D

Abstract

The mathematical simplicity of black holes, combined with their links to some of the most energetic events in the universe, means that black holes are key objects for fundamental physics and astrophysics. Until recently, it was generally believed that black holes in nature appear in two broad mass ranges: stellar-mass (M~3–20 M⊙), which are produced by the core collapse of massive stars, and supermassive (M~10 6–10 10 M⊙), which are found in the centers of galaxies and are produced by a still uncertain combination of processes. In the last few years, however, evidence has accumulated for an intermediate-mass class of black holes, with M~10 2–10 4 M⊙. If such objects exist they have important implications for the dynamics of stellar clusters, the formation of supermassive black holes, and the production and detection of gravitational waves. We review the evidence for intermediate-mass black holes and discuss future observational and theoretical work that will help clarify numerous outstanding questions about these objects.

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Metadata

Authors
COLEMAN MILLER, M., & COLBERT, E. J. M.
Venue
International Journal of Modern Physics D
Published
2004-01
Volume
13
Issue
01
Pages
1-64
ISSN
  • 0218-2718 (ISSN-L)
  • 1793-6594
OpenAlex
W2114133132
Cited by
443
References
165
FWCI
21.46
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: INTERMEDIATE-MASS BLACK HOLES. https://app.cochat.ai/papers/10.1142/s0218271804004426
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COLEMAN MILLER, M., & COLBERT, E. J. M. (2004). INTERMEDIATE-MASS BLACK HOLES. International Journal of Modern Physics D. https://doi.org/10.1142/s0218271804004426

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