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相关论文: Properties of warm absorbers in active galaxies

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Warm absorbers are an important new probe of the central region of active galaxies (AGN). Observing and modeling this component provides a wealth of information on the nature of the warm absorber itself, its relation to other components of…

天体物理学 · 物理学 2009-10-31 Stefanie Komossa , Dieter Breitschwerdt , Janek Meerschweinchen

We first provide a review of the properties of warm absorbers concentrating on what we have learned from ROSAT and ASCA. This includes dusty and dust-free warm absorbers, non-X-ray emission and absorption features of warm absorbers, and the…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa

Warm absorbers are an important new tool for investigating the conditions within the central regions of active galaxies. They have been observed in ~50% of the well-studied Seyfert galaxies and have also been detected in quite a number of…

天体物理学 · 物理学 2009-10-31 Stefanie Komossa , Jochen Greiner

We present a study of the properties of dusty warm absorbers and point to some important consequences for the resulting X-ray absorption spectra of AGN. Pronounced effects of the presence of dust in warm material are (i) an apparent…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Norbert Bade

We study the properties of warm absorbers in several active galaxies (AGN) and present new candidates, using ROSAT X-ray observations. Several aspects of the characteristics of warm absorbers are discussed, constraints on the density and…

天体物理学 · 物理学 2009-10-28 Stefanie Komossa , Henner Fink

IRAS13349+2438 was the first quasar suggested to host a warm absorber with internal dust. We obtained new HRI data for this object and derive constraints on the X-ray emitting region of IRAS13349+2438 by investigating its X-ray extent and…

天体物理学 · 物理学 2007-05-23 J. Siebert , S. Komossa , W. Brinkmann

X-ray spectroscopy of Seyfert 1 galaxies often reveal absorption edges resulting from photoionized gas along the line-of-sight to the central engine, the so-called warm absorber. I discuss how recent ASCA observations of warm absorber…

天体物理学 · 物理学 2007-05-23 C. S. Reynolds

We present a wide grid of models for the structure and transmission properties of warm absorbers in active galactic nuclei (AGN). Contrary to commonly used constant density models, our absorbing cloud is assumed to be under constant total…

天体物理学 · 物理学 2007-05-23 A. Rozanska , R. Goosmann , A. -M. Dumont , B. Czerny

We present evidence for X-ray absorption by ionized oxygen in ASCA spectra of the prototype infrared quasar IRAS 13349+2438. This powerful (2E46 erg/s) quasar was studied in detail with ROSAT, and the combination of the X-ray data and…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , S. Mathur , C. S. Reynolds , M. Elvis

Warm absorbers are an important new probe of the central regions of active galaxies. So far, they revealed their existence mainly in the soft X-ray spectral region. In observing and modeling this component, we can learn a lot about the…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa

Using spatially resolved, deprojected ROSAT PSPC spectra of 10 of the brightest cooling flow galaxies and groups with low Galactic column densities we have detected intrinsic absorption over energies ~0.4-0.8 keV in half of the sample.…

天体物理学 · 物理学 2009-10-31 David A. Buote

Recent {\it ASCA} observations confirm the presence of X-ray absorption due to partially ionized gas in many Seyfert 1 galaxies; the so-called warm absorber. Constraints on the location of the warm material are presented with the conclusion…

天体物理学 · 物理学 2015-06-24 C. S. Reynolds , A. C. Fabian

We present spatial, temporal and spectral analyses of ROSAT Position Sensitive Proportional Counter (PSPC) observations of the infrared loud quasar IRAS 13349+2438. IRAS 13349+2438 is the archetypal highly-polarized radio-quiet QSO and has…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , A. C. Fabian , K. A. Pounds

Observations of warm absorbers provided new ways to study the nuclear environments of AGNs. I discuss basic properties of warm absorbers and early developments with ROSAT, ASCA and HST observations. I briefly touch upon recent advances made…

天体物理学 · 物理学 2007-05-23 Smita Mathur

BeppoSAX observations of the high redshift (z=4.72) blazar GB 1428+4217 confirm the presence of a complex soft X-ray spectrum first seen with the ROSAT PSPC. Flattening below a rest frame energy of 5 keV can be accounted for by absorption…

天体物理学 · 物理学 2009-09-17 A. C. Fabian , A. Celotti , K. Iwasawa , G. Ghisellini

The unified picture of X-ray/UV absorbers offers an unique opportunity to probe the nuclear environment of AGNs. To test the unified absorber scenario and to understand the physical properties of the absorber we obtained the first UV…

天体物理学 · 物理学 2009-10-30 Smita Mathur , Belinda Wilkes , Martin Elvis

We report the detection of ionized absorption in the ASCA spectrum of the narrow-line Seyfert 1 galaxy IRAS 17020+4544. Subsequent optical spectropolarimetry revealed high polarization increasing from 3% in the red to 5% in the blue,…

天体物理学 · 物理学 2009-10-30 Karen M. Leighly , Laura E. Kay , Beverley J. Wills , D. Wills , Dirk Grupe

We have surveyed the optical linear polarimetric properties of 65 soft X-ray selected ROSAT Active Galactic Nuclei (AGN). Most of these sources show low polarization (<1%) and no optical reddening. This is in agreement with the X-ray…

天体物理学 · 物理学 2007-05-23 D. Grupe , Beverley J. Wills , D. Wills , Karen M. Leighly

We present results on the X-ray spectrum of the quasar PG 1114+445 from an ASCA observation performed in 1996 June, and a ROSAT observation performed 3 years earlier. We show good agreement between all the datasets can be obtained if the…

天体物理学 · 物理学 2009-10-30 I. M. George , K. Nandra , A. Laor , T. J. Turner , F. Fiore , H. Netzer , R. F. Mushotzky

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…

宇宙学与河外天体物理 · 物理学 2015-05-28 Shui-Nai Zhang , Qiu-Sheng Gu , Li Ji , Zhi-Xin Peng
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