A study of the correlation between the amplification of the Fe Kα line and the X-ray continuum of quasars due to microlensing

Astrophysical Journal

Volumn 637, Issue 2 I, 2006, Pages 620-630

  Popovic L C ^a,b   Jovanovic P ^a,b   Mediavilla, E ^c   Zakharov, A F ^d,e,f   Abajas, C ^c   Munoz J A ^c,g   Chartas, G ^h  

^a ASTRONOMICAL OBSERVATORY   (Serbia)

^b UNIVERSIDAD DIEGO PORTALES   (Chile)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^d INSTITUTE FOR THEORETICAL AND EXPERIMENTAL PHYSICS   (Russian Federation)

^e LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^f Isaac Newton Institute of Chile   (Russian Federation)

^g UNIVERSITY OF VALENCIA   (Spain)

^h PENNSYLVANIA STATE UNIVERSITY   (United States)

Author keywords

Gravitational lensing; X rays: galaxies

Indexed keywords

EID: 33144488273     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/498558     Document Type: Article

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