paper

A multi-wavelength study of nuclear activity and environment of a low power radio galaxy CTD 86

arXiv:1212.6171 · doi:10.1093/mnras/stt1531

Abstract

We present an X-ray study of the nuclear and extended emission of a nearby Fanaroff & Riley class I (FR-I) radio galaxy CTD 86 based on the \xmm{} observations. Two different components observed are : diffuse thermal emission from hot gas ($kT\sim 0.79\kev$, , extended over ), and unresolved nuclear emission exhibiting mild activity. The hot gaseous environment of CTD 86 is similar to that found in groups of galaxies or in bright early-type galaxies. No clear signatures of radio-lobe interaction with the diffuse hot gas is evident in this case. X-ray emission from the nucleus is well constrained by an intrinsically absorbed () power law () with $2-10\kev$ luminosity . We have measured the stellar velocity dispersion, $σ=182\pm8\kms$, for the CTD 86 and estimated a mass with . The low rate and high ratio suggest that the central engine of CTD 86 consists of a truncated accretion disk lacking a strong ionizing UV radiation and an inner hot flow producing the X-ray emission. The truncated disk is likely to be inclined with () such that our line of sight passes through the outer regions of a putative torus and thus results in high X-ray absorption. We have also identified two bright X-ray sources, SDSS J142452.11+263715.1 and SDSS J142443.78+263616.2, near CTD 86. SDSS J142452.11+263715.1 is a type 1 active galactic nucleus at and unabsorbed $0.3-10\kev$ X-ray luminosity , while SDSS J142443.78+263616.2 is probably a galaxy with an active nucleus.

19 pages, 3 Tables, 9 figures, Accepted for publication in MNRAS

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