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Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
Exploring the nature of the brightest hyper-luminous X-ray source
Astronomische Nachrichten, Volume 332, No. 4, Year 2011
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Description
The small subset of hyper-luminous X-ray sources with luminosities in excess of ~1041 erg s-1 are hard to explain without the presence of an intermediate mass black hole, as significantly super-Eddington accretion and/or very small beaming angles are required. The recent discovery of HLX-1, the most luminous object in this class with a record breaking luminosity of ~1042 erg s-1 in the galaxy ESO 243-49, therefore currently provides some of the strongest evidence for the existence of intermediate mass black holes. HLX-1 is almost an order of magnitude brighter than the other hyperluminous sources, and appears to exhibit X-ray spectral and flux variability similar to Galactic stellar mass black hole X-ray binaries. In this paper we review the current state of knowledge on this intriguing source and outline the results of multi-wavelength studies from radio to ultra-violet wavelengths, including imaging and spectroscopy of the recently identified optical counterpart obtained with the Very Large Telescope. These results continue to support an intermediate mass black hole in excess of 500 M⊙. © 2011 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.
Authors & Co-Authors
Farrell, Sean A.
United Kingdom, Leicester
University of Leicester
Servillat, Mathieu
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Wiersema, Klaas
United Kingdom, Leicester
University of Leicester
Barret, Didier
France, Toulouse
Université Fédérale Toulouse Midi-pyrénées
France, Toulouse
Institut de Recherche en Astrophysique et Planétologie Irap
Godet, Olivier
France, Toulouse
Université Fédérale Toulouse Midi-pyrénées
France, Toulouse
Institut de Recherche en Astrophysique et Planétologie Irap
Heywood, Ian
United Kingdom, Oxford
University of Oxford
MacCarone, Thomas J.
United Kingdom, Southampton
University of Southampton
Oates, Samantha R.
United Kingdom, Dorking
Ucl Mullard Space Science Laboratory
Webb, Natalie A.
France, Toulouse
Université Fédérale Toulouse Midi-pyrénées
France, Toulouse
Institut de Recherche en Astrophysique et Planétologie Irap
Statistics
Citations: 13
Authors: 9
Affiliations: 7
Identifiers
Doi:
10.1002/asna.201011507
ISSN:
15213994