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Related papers: Changing-look event in NGC 3516: continuum or obsc…

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We present echelle observations of the intrinsic UV absorption lines in the Seyfert galaxy NGC 4151, which were obtained with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope on 1999 July 19. The UV continuum…

We present evidence of flux variability, on both short (hours) and long (months) time scales of the Seyfert 2 galaxy NGC 7172. These results are based on the ASCA observation of NGC 7172 performed on May 1996. The source was detected at a…

Astrophysics · Physics 2009-10-30 M. Guainazzi , G. Matt , L. A. Antonelli , F. Fiore , L. Piro , S. Ueno

Two major challenges to unification schemes for active galactic nuclei (AGN) are the existence of Narrow-Line Seyfert 1s (NLS1s) and the existence of changing-look (CL) AGNs. AGNs can drastically change their spectral appearance in the…

Astrophysics of Galaxies · Physics 2019-07-09 Victor L. Oknyansky , Konstantin L. Malanchev , C. Martin Gaskell

We present an analysis of historical multi-wavelength emission of the Changing Look (CL) Active Galactic Nucleus (AGN) in NGC 2992, covering epochs ranging from 1978 to 2021, as well as new X-ray and optical spectra. The galaxy presents…

Significant variability in broad emission line strengths of active galactic nuclei (AGN) over months to years has been observed, often accompanied by intrinsic continuum changes. Such spectral variability challenges the traditional AGN…

Astrophysics of Galaxies · Physics 2025-07-22 Tek P. Adhikari , Santanu Mondal , Zhicheng He , Agata Rozanska , Krzysztof Hryniewicz

The X-ray spectra of two intermediate type Seyfert galaxies are investigated using ASCA observations separated by more than a year. Both NGC 4388 and ESO 103-G35 exhibit strong, narrow Fe K alpha line emission and absorption by cold neutral…

Astrophysics · Physics 2009-10-31 Karl Forster , Karen M. Leighly , Laura E. Kay

We report an intrinsic absorber with decreasing outflow velocity in the Seyfert 1 galaxy NGC 3783. This is the first detection of a change in radial velocity in an outflow associated with a Seyfert galaxy. These results are based on…

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 report on the changing-look nature of the active galactic nucleus (AGN) in the galaxy NGC 4156, as serendipitously discovered thanks to data acquired in 2019 at the Telescopio Nazionale Galileo (TNG) during a students' observing…

The short-term spectral variability of the narrow-line Seyfert 1 galaxy I Zwicky 1 (I Zw 1) as observed in an 85 ks XMM-Newton observation is discussed in detail. I Zw 1 shows distinct modes of variability prior to and after a flux dip in…

Astrophysics · Physics 2008-11-26 L. C. Gallo , W. N. Brandt , E. Costantini , A. C. Fabian

We report on the results of a three-year program of coordinated X-ray and optical monitoring of the narrow-line Seyfert 1 galaxy NGC 4051. The rapid continuum variations observed in the X-ray spectra are not detected in the optical,…

We studied the multiwavelength properties of NGC 3521, the Milky Way galaxy-twin, from UV- to radio, exploring the data from GALEX for UV-, SDSS for optical, 2MASS, WISE, MIPS (Spitzer) and PACS, SPIRE (Herschel) for IR-, and NRAO VLA for…

Astrophysics of Galaxies · Physics 2026-01-27 O. S. Pastoven , O. V. Kompaniiets , I. B. Vavilova , I. O. Izviekova

We discuss the results of a campaign to monitor spectral variations in the low-luminosity Seyfert~1 galaxy NGC~4593, at X-rays, ultraviolet, optical and near IR frequencies. The observations and data analysis have been described in a…

Astrophysics · Physics 2015-06-24 M. Santos-Lleo , J. Clavel , P. Barr , I. S. Glass , D. Pelat , B. M. Peterson , G. Reichert

We present a complete analysis of the hard X-ray (2-10 keV) properties of the Seyfert galaxy NGC 1365, based on a 60 ks XMM-Newton observation performed in January 2004. The two main results are: 1) We detect an obscuring cloud with…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 G. Risaliti , G. Miniutti , G. Fabbiano , M. Salvati , A. Baldi , V. Braito , S. Bianchi , G. Matt , J. Reeves , R. Soria , A. Zezas

We report on two Chandra observations, and a simultaneous Hubble Space Telescope ultraviolet observation, of the dwarf Seyfert 1 galaxy NGC 4395. Each Chandra observation had a duration of ~30 ks, with a separation of ~50 ks. The spectrum…

We report the discovery of the Narrow-Line Seyfert 1 galaxy Mkn 335 in an extremely low X-ray state. A comparison of Swift observations obtained in May and June/July 2007 with all previous X-ray observations between 1971 to 2006 show the…

Astrophysics · Physics 2009-11-13 Dirk Grupe , Stefanie Komossa , Luigi Gallo

This paper reports on two XMM-Newton observations of the Seyfert 1 Galaxy H0557-385 obtained in 2006, which show the source at an historical low flux state, more than a factor of 10 lower than a previous XMM-Newton look in 2002. The low…

Astrophysics · Physics 2009-11-13 A. L. Longinotti , S. Bianchi , L. Ballo , I. de la Calle , M. Guainazzi

We report the tentative detection of the modulation of a transient, redshifted Fe Kalpha emission feature in the X-ray spectrum of the Seyfert galaxy NGC3516. The detection of the spectral feature at 6.1 keV, in addition to a stable 6.4 keV…

Astrophysics · Physics 2009-09-17 K. Iwasawa , G. Miniutti , A. C. Fabian

The presence of an obscuring torus around the nucleus of Seyfert galaxies, as supposed in the popular unification scheme, can strongly modify the X--ray spectrum for both type 1 and 2 Seyfert galaxies. We find that if the torus is Compton…

Astrophysics · Physics 2015-06-24 Gabriele Ghisellini , Francesco Haardt , Giorgio Matt

The ISO-SWS infrared spectroscopic observations of the nucleus of Seyfert galaxy NGC4151, which are described in a companion paper, are used together with a compilation of UV to IR narrow emission line data to determine the spectral shape…