The ionized gas and nuclear environment in NGC 3783. IV. Variability and modeling of the 900 kilosecond Chandra spectrum

Astrophysical Journal

Volumn 599, Issue 2 I, 2003, Pages 933-948

  Netzer, Hagai ^a   Kaspi, Shai ^a   Behar, Ehud ^b   Brandt, W N ^c   Chelouche, Doron ^a   George, Ian M ^d,e   Crenshaw, D Michael ^f   Gabel, Jack R ^g   Hamann, Frederick W ^h   Kraemer, Steven B ^g   Kriss, Gerard A ^i,j   Nandra, Kirpal ^k   Peterson, Bradley M ^l   Shields, Joseph C ^m   Turner, T J ^d,e  

^a TEL AVIV UNIVERSITY   (Israel)

^b TECHNION ISRAEL INSTITUTE OF TECHNOLOGY   (Israel)

^c PENNSYLVANIA STATE UNIVERSITY   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

^f GEORGIA STATE UNIVERSITY   (United States)

^g CATHOLIC UNIVERSITY OF AMERICA   (United States)

^h 211 Bryant Space Science Center ^*  (United States)

ⁱ JOHNS HOPKINS UNIVERSITY   (United States)

^j AURA for the European Space Agency   (United States)

^k IMPERIAL COLLEGE LONDON   (United Kingdom)

^l OHIO STATE UNIVERSITY   (United States)

^m OHIO UNIVERSITY   (United States)

more..

Author keywords

Galaxies: active; Galaxies: individual (NGC 3783); Galaxies: nuclei; Galaxies: Seyfert; Techniques: spectroscopic; X rays: galaxies

Indexed keywords

EID: 0347931793     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/379508     Document Type: Review

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