The X-ray spectrum of the Seyfert I galaxy Markarian 766: Dusty warm absorber or relativistic emission lines?

Astrophysical Journal

Volumn 582, Issue 1 I, 2003, Pages 95-104

  Mason, K O ^a   Branduardi Raymont, G ^a   Ogle, P M ^b   Page, M J ^a   Puchnarewicz, E M ^a   Behar, E ^c   Cordova F A ^b   Davis, S ^b   Maraschi, L ^d   McHardy, I M ^e   O'Brien, P T ^f   Priedhorsky, W C ^g   Sasseen, T P ^b  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c Columbia University ^*  (United States)

^d INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^e UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^f UNIVERSITY OF LEICESTER   (United Kingdom)

^g LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

Accretion, accretion disks; Galaxies: individual (Markarian 766); Galaxies: Seyfert; Line: profiles; X rays: galaxies

Indexed keywords

EID: 0041761147     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/344562     Document Type: Article

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