XMM-Newton unveils the complex iron K α region of Mrk 279

Astronomy and Astrophysics

Volumn 512, Issue 4, 2010, Pages

  Costantini, E ^a   Kaastra, J S ^a,b   Korista, K ^c   Ebrero, J ^a   Arav, N ^d   Kriss, G ^e   Steenbrugge, K C ^f  

^a SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^b UTRECHT UNIVERSITY   (Netherlands)

^c WESTERN MICHIGAN UNIVERSITY   (United States)

^d VIRGINIA POLYTECHNIC INSTITUTE AND STATE UNIVERSITY   (United States)

^e STScI   (United States)

^f ST JOHN S COLLEGE   (United Kingdom)

Author keywords

Galaxies: individual: Mrk 279; Galaxies: Seyfert; Quasars: absorption lines; Quasars: emission lines; X rays: galaxies

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GALAXIES; GAS ABSORPTION; IRON COMPOUNDS; LUMINANCE;

ABSOLUTE LUMINOSITY; ACCRETION DISKS; BROAD LINE REGION; COLD GAS; COLUMN DENSITY; EMISSION FEATURES; ENERGY BAND; GALAXIES: INDIVIDUALS; GALAXIES: SEYFERT; GAUSSIANS; HIGHLY-IONIZED; OUTER LAYER; SEYFERTS; TWO-COMPONENT; TWO-LINE; X RAYS:GALAXIES; XMM-NEWTON; XMM-NEWTON OBSERVATIONS;

IONIZATION OF GASES;

EID: 77951520907     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912555     Document Type: Article

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