A strong and broad Fe line in the XMM-Newton spectrum of the new X-ray transient and black hole candidate XTEJ1652-453

Monthly Notices of the Royal Astronomical Society

Volumn 411, Issue 1, 2011, Pages 137-150

  Hiemstra, Beike ^a   Méndez, Mariano ^a   Done, Chris ^b   Trigo, María Díaz ^c   Altamirano, Diego ^d   Casella, Piergiorgio ^e  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b DURHAM UNIVERSITY   (United Kingdom)

^c EUROPEAN SPACE AGENCY   (Spain)

^d UNIVERSITY OF AMSTERDAM   (Netherlands)

^e UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Accretion, accretion discs; Black hole physics; Stars: individual: XTEJ1652 453; X rays: binaries

Indexed keywords

BLACK HOLES; GRAVITATION; STARS;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BLACK HOLE CANDIDATES; BLACK HOLE PHYSICS; SPECTRA'S; STAR: INDIVIDUAL: XTEJ1652-453; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY TRANSIENTS; X-RAYS: BINARIES; XMM-NEWTON;

POWER SPECTRUM;

EID: 78751684197     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.17661.x     Document Type: Article

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