A 3 dimensional diagnostic diagram for Seyfert 2s: probing X-ray absorption and Compton thickness
arXiv:astro-ph/9811074 · doi:10.1086/313202
Abstract
We present and discuss a "3-dimensional" diagnostic diagram for Seyfert2 galaxies obtained by means of X-ray and [OIII] data on a large sample of objects (reported in the Appendix). The diagram shows the Kalpha iron line equivalent width as a function of both the column density derived from the photoelectric cutoff and the 2-10 keV flux normalized to the [OIII] optical line flux (the latter corrected for extinction and assumed to be a true indicator of the source intrinsic luminosity). We find that the hard X-ray properties of type 2 objects depend on a single parameter, the absorbing column density along the line of sight,in accordance with the unified model. The diagram can be used to identify Compton thick sources and to isolate and study peculiar objects. From this analysis we have obtained a column density distribution of Seyfert 2 galaxies which is thought to be a good approximation of the real distribution. A large population of heavily absorbed objects is discovered, including many Compton thick candidates. Our results indicate that the mean Log Nh/cm^(-2)in type 2 Seyferts is 23.5 and that as much as 23-30% of sources have Nh > 10^24 cm^(-2).
33 pages, 3 figures, to be published in ApJ Supp
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- Embedded AGN and star formation in the central 80 pc of IC 3639
- X-ray long-term variations in the low-luminosity AGN NGC835 and its circumnuclear emission
- Properties of IR selected Active Galactic Nuclei
- SDSS-IV MaNGA: Identification and Multiwavelength Properties of Type-1 AGN in the DR15 sample
- The Complex X-ray Obscuration Environment in the Radio Loud Type 2 Quasar 3C 223
- Double-nucleus elliptical MCG-01-12-005 in an X-ray emitting cluster of galaxies
- The luminous infrared composite Seyfert 2 galaxy NGC 7679 through the [O III] 5007 emission line
- X-ray view of four high-luminosity Swift/BAT AGN: Unveiling obscuration and reflection with Suzaku
- On the origin of X-ray oxygen emission-lines in obscured AGN
- IC 485:a new candidate disk-maser galaxy at 100 Mpc distance. Milliarcsecond resolution study of the galaxy nucleus and of the megamaser
- The X-ray Nature of Nucleus in Seyfert 2 Galaxy NGC 7590
- Mkn 463 field observed by BeppoSAX
- Obscured Narrow-Line Seyfert 1 Galaxy Candidate Mrk 1388 with Nonthermal Jets
- A search for HO masers in 100 active dwarf galaxies
- The extragalactic nature of the serendipitous BeppoSAX source 2MASX J14585116-1652223
- The XMM-Newton hard band wide angle Survey
- Multi-wavelength properties of the high-energy bright Seyfert 1 galaxy IGR J18027-1455