Chandra/high energy transmission grating spectrometer spectroscopy of the Galactic black hole GX 339-4: A relativistic iron emission line and evidence for a seyfert-like warm absorber

Astrophysical Journal

Volumn 601, Issue 1 I, 2004, Pages 450-465

  Miller, J M ^a,b   Raymond, J ^a   Fabian, A C ^c   Homan, J ^d   Nowak, M A ^e   Wijnands, R ^f   Van Der Klis, M ^g   Belloni, T ^d   Tomick, J A ^h   Smith, D M ⁱ   Charles, P A ^j   Lewin, W H G ^e  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b NSF Astronomy and Astrophysics   (United States)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^e MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^f UNIVERSITY OF ST ANDREWS   (United Kingdom)

^g UNIVERSITY OF AMSTERDAM   (Netherlands)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF CALIFORNIA SANTA CRUZ   (United States)

^j UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

more..

Author keywords

Accretion, accretion disks; Black hole physics; Relativity stars: individual (GX 339 4, XTE J1650 500)

Indexed keywords

EID: 1642586477     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/380196     Document Type: Article

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