Compton Shoulder Diagnostics in Active Galactic Nuclei for Probing the Metalicity of the Obscuring Compton-Thick Tori
arXiv:1810.01088 · doi:10.3847/1538-4357/aae1fe
Abstract
We analyzed the spectral shape of the Compton shoulder around the neutral Fe-K line of the Compton-thick type II Seyfert nucleus of the Circinus galaxy. The characteristics of this Compton shoulder with respect to the reflected continuum and Fe-K line core intensity are a powerful diagnostics tool for analyzing the structure of the molecular tori, which obscure the central engine. We applied our Monte-Carlo-based X-ray reflection spectral model to the Chandra High Energy Transmission Grating data and successfully constrained the various spectral parameters independently, using only the spectral data only around the Fe-K emission line. The obtained column density and inclination angle are consistent with the previous observations and the Compton-thick type II Seyfert picture. In addition, we determined the metal abundance of the molecular torus for the case of the smooth and clumpy torus to be 1.75 and 1.740.16 solar abundance, respectively. Such slightly over-solar abundance can be useful information for discussing the star formation rate in the molecular tori of active galactic nuclei.
8 pages, 3 figures, 1 table, accepted for publication in The Astrophysical Journal
References in corpus (7)
- AGN Dusty Tori: I. Handling of Clumpy Media
- Emission-line Diagnostics of Low Metallicity AGN
- Radiative Transfer Modeling of Three-Dimensional Clumpy AGN Tori and its Application to NGC 1068
- The 2-79 keV X-ray Spectrum of the Circinus Galaxy with NuSTAR, XMM-Newton and Chandra: a Fully Compton-Thick AGN
- Starbursts and torus evolution in AGN
- Sensitivity of the Fe K-alpha Compton shoulder to the geometry and variability of the X-ray illumination of cosmic objects
- Suzaku observation of the Phoenix Galaxy
Cited by in corpus (7)
- X-Ray Spectral Model from Clumpy Torus and Its Application to Circinus Galaxy
- X-ray radiative transfer in full 3D with SKIRT
- X-ray Constraint on Location of AGN Torus in Circinus Galaxy
- X-ray Simulations of Polar Gas in Accreting Supermassive Black Holes
- NuSTAR observations of a heavily X-ray obscured AGN in the dwarf galaxy J144013+024744
- Ray-tracing simulations of the Soft X-ray Scattered Emission in obscured Active Galactic Nuclei
- The FeK Compton shoulder in accreting Supermassive Black Holes