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• W2081569785 abstract "We present X-ray imaging spectroscopy of the extremely luminous infrared galaxy IRAS 09104+4109 (z = 0.442) obtained with the Chandra X-ray Observatory. With the arcsec resolution of Chandra, an unresolved source at the nucleus is separated from the surrounding cluster emission. A strong iron K line at 6.4 keV on a very hard continuum is detected from the nuclear source, rendering IRAS 09104+4109 the most distant reflection-dominated X-ray source known. Combined with the BeppoSAX detection of the excess hard X-ray emission, it provides further strong support for the presence of a hidden X-ray source of quasar luminosity in this infrared galaxy. Also seen is a faint linear structure to the north, which coincides with the main radio jet. An X-ray deficit in the corresponding region suggests an interaction between the cluster medium and the jet driven by the active nucleus." @default.
• W2081569785 created "2016-06-24" @default.
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• W2081569785 date "2001-02-11" @default.
• W2081569785 modified "2023-10-05" @default.
• W2081569785 title "Chandra detection of reflected X-ray emission from the type 2 QSO in IRAS 09104+4109" @default.
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• W2081569785 doi "https://doi.org/10.1046/j.1365-8711.2001.04236.x" @default.
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