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相关论文: A unique X-ray unabsorbed Seyfert 2 galaxy IRAS F0…

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We present the results of a Suzaku monitoring campaign of the Seyfert 2 galaxy, NGC7582. The source is characterized by very rapid (on timescales even lower than a day) changes of the column density of an inner absorber, together with the…

We present an X-ray spectral analysis of a sample of 8 bona-fide Seyfert 2 galaxies, selected on the basis of their high $[OIII]\lambda5007$ flux, from the Ho et al. (1997) spectroscopic sample of nearby galaxies. We find that, in general,…

天体物理学 · 物理学 2008-11-26 A. Pappa , I. Georgantopoulos , G. C. Stewart , A. L. Zezas

IRAS 00521$-$7054 is the first Seyfert 2 in which the presence of an extremely large Fe K$\alpha$ line has been claimed. We report here on the analysis of a 100 ks Suzaku observation of the source. We confirm the existence of a very strong…

高能天体物理现象 · 物理学 2015-06-22 Claudio Ricci , Fumie Tazaki , Yoshihiro Ueda , Stephane Paltani , Rozenn Boissay , Yuichi Terashima

We present a Suzaku observation of the dwarf Seyfert galaxy NGC4395 with an estimated black hole mass of ~10^5 Msun. Rapid and strong X-ray variability with an rms amplitude of ~60 per cent is observed in the 0.4-10 keV band with the XIS…

宇宙学与河外天体物理 · 物理学 2016-03-02 K. Iwasawa , Y. Tanaka , L. C. Gallo

I present ASCA observations of IRAS00317-2142, the most luminous (Lx~10^43 erg s-1 0.1-2 keV) of the 'composite' class of galaxies. This enigmatic class of objects presents narrow-emission line optical spectra classifying these galaxies as…

天体物理学 · 物理学 2009-10-31 I. Georgantopoulos

We present a study of the variations in the absorbing column density of 25 X-ray defined Seyfert 2 galaxies, as inferred from hard X-ray observations, on timescales from months to several years. We show that a significant variation of N$_H$…

天体物理学 · 物理学 2009-11-06 G. Risaliti , M. Elvis , F. Nicastro

We present an analysis of six 12 um selected Seyfert 2 galaxies that have been reported to be unabsorbed in the X-ray. By comparing the luminosities of these galaxies in the mid-IR (12um), optical ([O III]) and hard X-ray (2-10 keV), we…

天体物理学 · 物理学 2009-11-13 Murray Brightman , Kirpal Nandra

The state of the matter that is obscuring a small circumnuclear region in AGN can be probed by observations of its broad emission lines. Infrared lines are particularly useful since they penetrate significant columns of obscuring matter,…

天体物理学 · 物理学 2009-11-07 D. Lutz , R. Maiolino , A. F. M. Moorwood , H. Netzer , S. J. Wagner , E. Sturm , R. Genzel

Using the 3XMM catalogue of serendipitous X-ray sources, and the SDSS-DR9 spectroscopic catalogue, we have obtained a new sample of X-ray selected narrow emission line galaxies. The standard optical diagnostic diagram and selection by hard…

高能天体物理现象 · 物理学 2014-09-05 Estelle Pons , Mike G. Watson

We present Suzaku observations of five hard X-ray selected nearby Seyfert 2 galaxies. All the sources were clearly detected with the pin Hard X-ray Detector up to several tens of keV, allowing for a fairly good characterization of the…

高能天体物理现象 · 物理学 2015-05-19 A. Comastri , K. Iwasawa , R. Gilli , C. Vignali , P. Ranalli , G. Matt , F. Fiore

We present a sample of 17 type 2 Seyfert galaxies which have an X-ray column density lower than 10^{22} cm^{-2}. The Compton thin nature of these sources is strongly suggested by isotropic indicators. We estimate the fraction of these…

天体物理学 · 物理学 2009-11-07 Francesca Panessa , Loredana Bassani

We present ROSAT HRI and ASCA observations of the well known ULIRG IRAS19254-7245 (the Superantennae). The object is not detected by ROSAT yielding a 3\sigma upper limit of L_x ~8x10^{41} erg/s in the 0.1-2 keV band. However, we obtain a…

天体物理学 · 物理学 2009-10-31 A. Pappa , I. Georgantopoulos , G. C. Stewart

We report on the first Suzaku observation of IGR J16318-4848, the most extreme example of a new group of highly absorbed X-ray binaries that have recently been discovered by the International Gamma-Ray Astrophysics Laboratory INTEGRAL. The…

高能天体物理现象 · 物理学 2015-05-14 L. Barragán , J. Wilms , K. Pottschmidt , M. A. Nowak , I. Kreykenbohm , R. Walter , J. A. Tomsick

We systematically analyzed the high-quality Suzaku data of 88 Seyfert galaxies. We obtained a clear relation between the absorption column density and the equivalent width of the 6.4 keV line above 10$^{23}$ cm$^{-2}$, suggesting a…

ASCA X-ray spectral analysis of the Seyfert 2 galaxy IRAS 04575-7537 is presented. The main result is the presence of a significant iron edge at a rest energy of 7.13^+0.21_-0.16 keV. The spectrum is flat (Gamma = 1.5) with a substantial…

天体物理学 · 物理学 2007-05-23 C. Vignali , A. Comastri , G. M. Stirpe , M. Cappi , G. G. C. Palumbo , M. Matsuoka , G. Malaguti , L. Bassani

We use hard X-ray data for an "optimal" sample of Seyfert 2 galaxies to derive the distribution of the gaseous absorbing column densities among obscured active nuclei in the local Universe. Of all Seyfert 2 galaxies in the sample, 75% are…

天体物理学 · 物理学 2009-10-31 G. Risaliti , R. Maiolino , M. Salvati

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…

A sample of X-ray and optically selected narrow emission-line galaxies (769 sources) from the 3XMM catalogue cross-correlated with SDSS (DR9) catalogue has been studied. Narrow-emission line active galactic nuclei (AGN; type-2) have been…

高能天体物理现象 · 物理学 2016-10-19 Estelle Pons , Mike G. Watson

We present a detailed analysis of the X-ray spectrum of the Seyfert 2 galaxy NGC454E, belonging to the interacting system NGC454. Observations performed with Suzaku, XMM-Newton and Swift allowed us to detect a dramatic change in the…

宇宙学与河外天体物理 · 物理学 2016-10-26 Elena Marchese , Valentina Braito , Roberto Della Ceca , Alessandro Caccianiga , Paola Severgnini

The new $XMM-Newton$ data of seven Seyfert 2 galaxies with optical spectropolarimetric observations are presented. The analysis of 0.5 -- 10 keV spectra shows that all four Seyfert 2 galaxies with polarized broad lines (PBLs) are absorbed…

天体物理学 · 物理学 2009-11-13 X. W. Shu , J. X. Wang , P. Jiang
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