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Cited by 508

The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.

An intermediate-mass black hole of over 500 solar masses in the galaxy ESO 243-49

Open access
Farrell, Sean A., Webb, Natalie A., Barret, Didier, Godet, Olivier, Rodrigues, Joana M.·2009·Nature

Abstract

Ultraluminous X-ray sources are extragalactic objects located outside the nucleus of the host galaxy with bolometric luminosities exceeding 1039 erg s-1. These extreme luminosities—if the emission is isotropic and below the theoretical (Eddington) limit, where the radiation pressure is balanced by the gravitational pressure—imply the presence of an accreting black hole with a mass of ∼102–105 solar masses (). The existence of such intermediate-mass black holes is in dispute, and though many candidates have been proposed, none are widely accepted as definitive. Here we report the detection of a variable X-ray source with a maximum 0.2–10 keV luminosity of up to 1.1 × 1042 erg s-1 in the edge-on spiral galaxy ESO 243-49, with an implied conservative lower limit for the mass of the black hole of ∼500.

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Crossref · 10.1038/nature08083

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Metadata

Authors
Farrell, S. A., Webb, N. A., Barret, D., Godet, O., & Rodrigues, J. M.
Venue
Nature
Published
2009-07
Volume
460
Issue
7251
Pages
73-75
ISSN
  • 0028-0836 (ISSN-L)
  • 1476-4687
OpenAlex
W2055832107
Cited by
508
References
14
FWCI
14.39
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: An intermediate-mass black hole of over 500 solar masses in the galaxy ESO 243-49. https://app.cochat.ai/papers/10.1038/nature08083
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Farrell, S. A., Webb, N. A., Barret, D., Godet, O., & Rodrigues, J. M. (2009). An intermediate-mass black hole of over 500 solar masses in the galaxy ESO 243-49. Nature. https://doi.org/10.1038/nature08083

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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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