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- W2094080342 abstract "We present a new Suzaku observation of the obscured AGN in NGC 1365, revealing an unexpected excess of X-rays above 20 keV of at least a factor ~2 with respect to the extrapolation of the best-fitting 3-10 keV model. Additional Swift-BAT and Integral-IBIS observations show that the 20-100 keV is concentrated within ~1.5 arcmin from the center of the galaxy, and is not significantly variable on time scales from days to years. A comparison of this component with the 3-10 keV emission, which is characterized by a rapidly variable absorption, suggests a complex structure of the circumnuclear medium, consisting of at least two distinct components with rather different physical properties, one of which covering >80% of the source with a column density NH~3-4x10^24 cm^(-2). An alternative explanation is the presence of a double active nucleus in the center of NGC 1365." @default.
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- W2094080342 date "2009-10-07" @default.
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- W2094080342 title "A STRONG EXCESS IN THE 20-100 keV EMISSION OF NGC 1365" @default.
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- W2094080342 doi "https://doi.org/10.1088/0004-637x/705/1/l1" @default.
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