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

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 ($kT\sim 0.79\text{kev}$, $n_e\sim {10}^{-3}\mathrm{c}{\mathrm{m}}^{-3}$, $L_X \sim 5\times10^{42}{\rm erg s^{-1}}$extendedover$\sim 186{\rm kpc}$), 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 ($N_H \sim 5.9\times10^{22}{\rm cm^{-2}}$)powerlaw($\Gamma \sim 1.5$)with$2-10\kev$luminosity$L_X \sim 2.1\times10^{42}{\rm erg s^{-1}}$. We have measured the stellar velocity dispersion, $\sigma =182\pm 8\text{kms}$, for the CTD 86 and estimated a mass $M_{BH}\sim 9\times {10}^7{\mathrm{M}}_{\odot }$ with $L_{bol}/L_{Edd} \sim 4\times10^{-3}$\mathrm{.}Thelow$L_{bol}/L_{Edd}$rateandhigh$L_X/L_{[O III]}$ 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 ($i\sim {40}^{\circ }-{50}^{\circ }$) 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 $z=0.3761$ and unabsorbed $0.3-10\text{kev}$ X-ray luminosity $L_X\sim 8\times {10}^{43}\mathrm{e}\mathrm{r}\mathrm{g}{\mathrm{s}}^{-1}$, while SDSS J142443.78+263616.2 is probably a galaxy with an active nucleus.