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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,…

Astrophysics · Physics 2008-11-26 A. Pappa , I. Georgantopoulos , G. C. Stewart , A. L. Zezas

We present results on the Seyfert 2 galaxy NGC4388 in the Virgo cluster observed with ASCA during its PV phase. The 0.5-10 keV X-ray spectrum consists of multiple components; (1) a continuum component heavily absorbed by a column density NH…

Astrophysics · Physics 2015-06-24 K. Iwasawa , A. C. Fabian , S. Ueno , H. Awaki , Y. Fukazawa , K. Matsushita , K. Makishima

We present the analysis of three XMM observations of the Seyfert 2 galaxy NGC 7590. The source was found to have no X-ray absorption in the low spatial resolution ASCA data. The XMM observations provide a factor of 10 better spatial…

High Energy Astrophysical Phenomena · Physics 2010-09-21 X. W. Shu , T. Liu , J. X. Wang

We obtained observations of NGC 4639 with ASCA in order to investigate its mildly active Seyfert 1 nucleus at hard X-ray energies. Koratkar et al. (1995) have previously shown that the nucleus is a pointlike source in the ROSAT soft X-ray…

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…

Astrophysics · Physics 2009-11-13 Murray Brightman , Kirpal Nandra

We present two Rossi Xray Timing Explorer (RXTE) PCA observations of the type~2 Seyfert galaxy NGC 4388 caught in an unusual low X-ray absorption state. The observations were triggered by a detection in the 1.5-3 keV band of the RXTE…

Astrophysics · Physics 2009-11-10 Martin Elvis , G. Risaliti , F. Nicastro , J. M. Miller , F . Fiore , S. Puccetti

We present the result of the Chandra high-resolution observation of the Seyfert~2 galaxy NGC 7590. This object was reported to show no X-ray absorption in the low-spatial resolution ASCA data. The XMM observations show that the X-ray…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Xinwen Shu , Junxian Wang , Teng Liu , Wei Zheng

ASCA observations of the Seyfert 2 galaxy NGC 7582 revealed it was highly variable on the timescale of $\sim2\times10^4$ s in the hard X-ray (2-10 keV) band, while the soft X-ray (0.5-2 keV) flux remained constant during the observations.…

Astrophysics · Physics 2015-06-24 S. -J. Xue , C. Otani , T. Mihara , M. Cappi , M. Matsuoka

We report the detection of an absorbed central X-ray source and its strong, rapid variability in NGC4395, the least luminous Seyfert nucleus known. The X-ray source exhibits a number of flares with factors of 3-4 flux changes during a half…

Astrophysics · Physics 2009-09-17 K. Iwasawa , A. C. Fabian , O. Almaini , P. Lira , A. Lawrence , K. Hayashida , H. Inoue

XMM-Newton observed the Seyfert 1.9 galaxy NGC 4258 in December 2000. At energies above 2 keV a hard nuclear point source is resolved that can be fitted by a highly absorbed power-law spectrum (NH = (8.0+-0.4)x10^22 cm^-2, photon index…

Astrophysics · Physics 2009-11-07 W. Pietsch , A. M. Read

Results from BeppoSAX observations of Compton--thick Seyfert 2 galaxies are summarized and reviewed, and their general properties derived and discussed. In five out of the seven observed sources, the nucleus is directly visible at high…

Astrophysics · Physics 2016-08-30 G. Matt , A. C. Fabian , M. Guainazzi , K. Iwasawa , L. Bassani , G. Malaguti

We present the results of a 17 ks Chandra observation of the nearby dwarf spiral galaxy NGC 4395, focusing on the X-ray properties of the moderate-mass black hole that resides in its nucleus. Chandra affords the first high-quality,…

Astrophysics · Physics 2007-05-23 E. C. Moran , M. Eracleous , K. M. Leighly , G. Chartas , A. V. Filippenko , L. C. Ho , P. R. Blanco

We derive the spectral energy distribution (SED) of the nucleus of the Seyfert galaxy NGC4565. Despite its classification as a Seyfert2, the nuclear source is substantially unabsorbed. The absorption we find from Chandra data (N_H=2.5 X…

Astrophysics · Physics 2008-11-26 M. Chiaberge , R. Gilli , F. D. Macchetto , W. B. Sparks

We present the results of a 17 ks Chandra ACIS-S observation of the nearby dwarf spiral galaxy NGC 4395. Chandra affords the first high-quality, broadband X-ray detection of the active nucleus of this object that is uncontaminated by nearby…

We present an analysis of the time-averaged spectrum of the Seyfert-2 active galaxy NGC 4388, obtained by NICER. The intrinsic strength of the reflection spectrum in NGC 4388, the large collecting area and favorable pass band of NICER, and…

High Energy Astrophysical Phenomena · Physics 2019-11-06 J. M. Miller , E. Kammoun , R. M. Ludlam , K. Gendreau , Z. Arzoumanian , E. Cackett , F. Tombesi

The first X-ray observation of the Seyfert 2 galaxy NGC5252 is reported. ASCA collected $\sim 4000$ photons/detector enough to perform an accurate spectral analysis of this source. The luminosity of NGC5252 is L$_{\rm X}$(0.7-10 keV)…

Astrophysics · Physics 2009-10-28 M. cappi , T. Mihara , M. Matsuoka , W. Brinkmann , M. A. Prieto , G. G. C. Palumbo

We report sub arc-second resolution X-ray imaging-spectroscopy of the archetypal type 2 Seyfert galaxy NGC 1068 with the Chandra X-ray Observatory. The observations reveal the detailed structure and spectra of the 13 kpc-extent nebulosity…

Astrophysics · Physics 2009-11-06 A. J. Young , A. S. Wilson , P. L. Shopbell

We analyze recent simultaneous Chandra/RXTE observations of the Seyfert 2 galaxy NGC 4945. The unprecedented spatial resolution of Chandra means we are able to separate the spectra of the nucleus, starburst and superwind regions, while the…

Astrophysics · Physics 2009-11-07 Chris Done , Greg M. Madejski , Piotr T. Zycki , Lincoln J. Greenhill

We present the Chandra imaging and spectral analysis of NGC 4968, a nearby (z = 0.00986) Seyfert 2 galaxy. We discover extended ($\sim$1 kpc) X-ray emission in the soft band (0.5 - 2 keV) that is neither coincident with the narrow line…

X-ray unabsorbed Seyfert 2 galaxies appear to have X-ray absorption column densities that are too low (NH < 10^22 cm-2) to explain the absence of broad emission lines in their optical spectra, challenging the standard AGN unification model.…

High Energy Astrophysical Phenomena · Physics 2011-05-25 Xing-Xing Huang , Jun-Xian Wang , Ying Tan , Huan Yang , Ya-Fang Huang
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