Arakelian 564: An XMM-Newton view

Monthly Notices of the Royal Astronomical Society

Volumn 347, Issue 3, 2004, Pages 854-860

  Vignali, Cristian ^a,b   Brandt, W N ^a   Boller, Th ^c   Fabian, A C ^d   Vaughan, Simon ^d,e  

^a PENNSYLVANIA STATE UNIVERSITY   (United States)

^b OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^e UNIVERSITY OF LEICESTER   (United Kingdom)

Author keywords

Galaxies: active; Galaxies: individual: Ark 564; Galaxies: Seyfert; X rays: galaxies

Indexed keywords

POWER SPECTRAL DENSITY;

BLACKBODY COMPONENTS; GALAXIES ACTIVE; GALAXIES: INDIVIDUAL: ARK 564; GALAXY:SEYFERT; NARROW LINES; POWER-LAW; SEYFERTS; X-RAYS: GALAXIES; XMM-NEWTON; XMM-NEWTON OBSERVATIONS;

GALAXIES;

EID: 1642559259     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07269.x     Document Type: Article

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