A Chandra view of the clumpy reflector at the heart of the Circinus galaxy

Abstract

We present a spectral and imaging analysis of the X-ray reflecting structure at the heart of the Circinus galaxy, investigating the innermost regions surrounding the central black hole. By studying an archival 200 ks Chandra ACIS-S observation, we are able to image the extended clumpy structure responsible for both cold reflection of the primary radiation and neutral iron Ka line emission. We measure an excess of the equivalent width of the iron Ka line which follows an axisymmetric geometry around the nucleus on a hundred pc scale. Spectra extracted from different regions confirm a scenario in which the dominant mechanism is the reflection of the nuclear radiation from Compton-thick gas. Significant differences in the equivalent width of the iron Ka emission line (up to a factor of 2) are found. It is argued that these differences are due to different scattering angles with respect to the line of sight rather than to different iron abundances.

6 pages, 4 figures, accepted for publication on MNRAS

References in corpus (4)

• AGN Dusty Tori: I. Handling of Clumpy Media
• The Large-Scale Atomic and Molecular Gas in the Circinus Galaxy
• Shocks, Seyferts and the SNR connection: a Chandra observation of the Circinus galaxy
• On Iron Enrichment, Star Formation, and Type Ia Supernovae in Galaxy Clusters

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