An intense soft excess and evidence for light bending in the luminous narrow-line quasar PHL 1092

Monthly Notices of the Royal Astronomical Society

Volumn 352, Issue 3, 2004, Pages 744-752

  Gallo, L C ^a   Boller, Th ^a   Brandt, W N ^b   Fabian, A C ^c   Grupe, D ^d  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d OHIO STATE UNIVERSITY   (United States)

Author keywords

Galaxies: active; Galaxies: individual: PHL 1092; Galaxies: nuclei; X rays: galaxies

Indexed keywords

ABSORPTION SPECTROSCOPY; BLACK HOLES; GRAVITATION; LIGHT; STARS;

GALAXIES ACTIVE; GALAXIES: INDIVIDUALS; GALAXIES:NUCLEI; GALAXY: INDIVIDUAL: PHL 1092; LIGHT CURVES; LIGHT-BENDING; NARROW LINES; ULTRA-VIOLET LIGHT; ULTRAVIOLET LIGHTS; X-RAYS: GALAXIES;

GALAXIES;

EID: 4043107834     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08003.x     Document Type: Article

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