Tracking the Complex Absorption in NGC 2110 with Two Suzaku Observations
arXiv:1403.1904 · doi:10.1088/0004-637X/786/2/126
Abstract
We present spectral analysis of two Suzaku observations of the Seyfert 2 galaxy, NGC 2110. This source has been known to show complex, variable absorption which we study in depth by analyzing these two observations set seven years apart and by comparing to previously analyzed observations with the XMM-Newton and Chandra observatories. We find that there is a relatively stable, full-covering absorber with a column density of ~3 cm, with an additional patchy absorber that is likely variable in both column density and covering fraction over timescales of years, consistent with clouds in a patchy torus or in the broad line region. We model a soft emission line complex, likely arising from ionized plasma and consistent with previous studies. We find no evidence for reflection from an accretion disk in this source with no contribution from relativistically broadened Fe Ka line emission nor from a Compton reflection hump.
Accepted to ApJ: March, 2014
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- The Seyfert 2 galaxy NGC 2110: hard X-ray emission observed by NuSTAR and variability of the iron K line
- Application of X-Ray Clumpy Torus Model (XCLUMPY) to 10 Obscured Active Galactic Nuclei Observed with Suzaku and NuSTAR
- AGN X-ray irradiation of CO gas in NGC 2110 revealed by and ALMA
- An X-ray variable absorber within the Broad Line Region in Fairall 51
- X-ray Photons in the CO 2-1 'Lacuna' of NGC 2110
- The NuSTAR View of the Seyfert 2 Galaxy NGC 4388