Radio emission from an ultraluminous x-ray source

Science

Volumn 299, Issue 5605, 2003, Pages 365-367

  Kaaret, Philip ^a   Corbel, Stephane ^b   Prestwich, Andrea H ^a   Zezas, Andreas ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITÉ PARIS DESCARTES   (France)

Author keywords

[No Author keywords available]

Indexed keywords

GALAXIES; RADIATION; X RAYS;

BLACK HOLES; RADIO EMISSIONS;

ATOMIC PHYSICS;

ASTRONOMY; RADIO WAVE; X-RAY;

ARTICLE; ASTRONOMY; ENERGY; LIGHT; LUMINANCE; OPTICS; PRIORITY JOURNAL; RADIATION; TELECOMMUNICATION; X RAY;

EID: 0346981996     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1079610     Document Type: Article

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43. We thank M. Georganopoulos for explaining the details of his model, the Chandra X-Ray Observatory team for carrying out the observations, M. Garcia and A. Kong for useful comments, J. Reynolds and T. Tzioumis for discussions of ATCA position uncertainties, and the Aspen Center for Physics where part of this work was carried out. Supported in part by a NASA Long-Term Space Astrophysics grant and a Chandra grant. We made use of NASA's High-Energy Astrophysics Science Archive Research Center. The Australia Telescope is funded by the Commonwealth of Australia for operation as a National Facility managed by the Commonwealth Scientific and Industrial Research Organisation.