Serendipitous discovery of warm absorbers in the Seyfert 2 galaxy IRAS 18325-5926
| Autor: | Zhi-Xin Peng, Shui-Nai Zhang, Li Ji, Qiusheng Gu |
|---|---|
| Rok vydání: | 2011 |
| Předmět: |
Physics
Cosmology and Nongalactic Astrophysics (astro-ph.CO) Active galactic nucleus Line-of-sight Astrophysics::High Energy Astrophysical Phenomena FOS: Physical sciences Astronomy and Astrophysics Quasar Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Redshift Galaxy Spectral line Space and Planetary Science Outflow Astrophysics::Galaxy Astrophysics Astrophysics - Cosmology and Nongalactic Astrophysics Line (formation) |
| Zdroj: | Research in Astronomy and Astrophysics. 11:1171-1184 |
| ISSN: | 1674-4527 |
| DOI: | 10.1088/1674-4527/11/10/006 |
| Popis: | Warm absorption is a common phenomenon in Seyfert 1s and quasars, but rare in Seyfert 2s. In this paper, we report the detection of warm absorbers with high energy resolution in the Seyfert 2 galaxy IRAS 18325-5926 for the first time with Chandra HETGS spectra. An intrinsic absorbing line system with an outflow velocity ~400 km/s was found, which is contributed by two warm absorbers with FWHM of 570 km/s and 1360 km/s, respectively. The two absorbers were adjacent, and doing a transverse motion across our line of sight. We constrained the distance of the absorbers to a small value, suggesting that the absorbers may originate from the highly ionized accretion disk wind. The perspective of this type 2 Seyfert provides the best situation to investigate the vertical part of the funnel-like outflows. Another weak absorbing line system with zero redshift was also detected, which could be due to Galactic absorption with very high temperature, or an intrinsic outflow with very high velocity ~6000 km/s. Comment: 14 pages, 10 figures |
| Databáze: | OpenAIRE |
| Externí odkaz: |
|