2009MNRAS.395L...1B

We report on the identification of the X/soft γ-ray source AX J183039-1002 detected with ASCA and INTEGRAL/IBIS. The source, which has an observed 20-100 keV flux of ∼8.6x10^–11 erg/cm2/s, is inside a diffuse radio supernova remnant (SNR) and is spatially coincident with a compact radio source. We analysed archival Chandra and XMM-Newton observations in order to identify the ASCA/INTEGRAL source. A point-like Chandra X-ray object was found to be positionally coincident with the compact radio source and within the error circle of the ASCA and INTEGRAL sources. Although the association of a compact radio/X-ray source with a radio SNR could be indicative of a pulsar wind nebula (PWN), the XMM-Newton X-ray spectrum is compatible with an absorbed, Seyfert-2 like active galactic nucleus, since it provides evidence for an iron emission line of ∼1 keV equivalent width; furthermore the X-ray source spectrum is similar to that of other Compton thick AGN where the ≲2 keV data are associated to a warm reflector and the ≳10 keV one to a cold reflector.