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X-Ray States and Radio Emission in the Black Hole Candidate XTE J1550-564 (2001)

Abstract
THE ASTROPHYSICAL JOURNAL June The American Astronomical Society All rights reserved Printed A RAY STATES AND RADIO EMISSION THE BLACK HOLE CANDIDATE XTE CORBEL AND KAARET Harvard Smithsonian Center for Astrophysics Garden Street Cambridge corbel head cfa harvard edu JAIN AND BAILYN Department Astronomy Yale University Box New Haven FENDER Astronomical Institute Anton Pannekoek University Amsterdam and Center for High Energy Astrophysics Kruislaan Amsterdam Netherlands TOMSICK AND KALEMCI Center for Astrophysics and Space Sciences Mail Stop University California San Diego Jolla MCINTYRE Australia Telescope National Facility Box Epping NSW Australia CAMPBELL WILSON School Physics University Sydney Sydney NSW Australia MILLER Center for Space Research Massachusetts Institute Technology Vassar Street Cambridge AND MCCOLLOUGH Universities Space Research Association Huntsville Received November accepted February ABSTRACT report radio and ray observations the black hole candidate BHC XTE performed during its ray outburst Observations were conducted with the Australia Telescope Compact Array and allowed sample the radio behavior XTE the ray low hard and intermediate very high states observed optically thin radio emission from XTE days after transition intermediate very high state but observed radio emission days later while XTE was still the intermediate very high state the low hard state XTE detected with inverted radio spectrum The radio emission the low hard state most likely ori

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Repository Publications of the Universiteit van Amsterdam (Netherlands)
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Type Article / Letter to the editor