X-ray states and radio emission in the black hole candidate XTE j1550-564

Astrophysical Journal

Volumn 554, Issue 1 PART 1, 2001, Pages 43-48

  Corbel, S ^a,i   Kaaret, P ^a   Jain, R K ^b   Bailyn, C D ^b   Fender, R P ^c   Tomsick, J A ^d   Kalemci, E ^d   Mcintyre, V ^e   Campbell Wilson, D ^f   Miller, J M ^g   Mccollough, M L ^h  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b YALE UNIVERSITY   (United States)

^c Center for High Energy Astrophysics   (Netherlands)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e CSIRO   (Australia)

^f UNIVERSITY OF SYDNEY   (Australia)

^g MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^h UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

ⁱ CEA SACLAY   (France)

Author keywords

Accretion, accretion disks; Black hole physics; Radio continuum: stars; Stars: individual (XTE J1550 564); X rays: stars

Indexed keywords

EID: 18044404330     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/321364     Document Type: Article

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