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Related papers: Rapid N_H Changes in NGC 4151

200 papers

We present Chandra X-ray observations of the nearby Seyfert 1.5 galaxy NGC 4151. The images show the extended soft X-ray emission on the several hundreds of pc scale with better sensitivity than previously obtained. The spectrum of the…

Astrophysics · Physics 2009-11-07 Y. Yang , A. S. Wilson , P. Ferruit

Observations of the C IV and Mg II absorption lines in the Seyfert 1 galaxy NGC 4151 obtained with the GHRS in October 1994 are presented. The data from the STScI archive show multiple broad and narrow components in both species. In…

Astrophysics · Physics 2007-05-23 Gerard A. Kriss

We report on a study of forbidden emission-line spectrum of nearby Seyfert 1.5 galaxy NGC 4151 based on the high-resolution (R ~ 45,000) optical spectrum obtained by using the High Dispersion Spectrograph boarded on the Subaru Telescope.…

Astrophysics · Physics 2009-11-07 Tohru Nagao , Takashi Murayama , Yasuhiro Shioya , Yoshiaki Taniguchi

We present the results of ultraviolet spectral monitoring of the Seyfert galaxy NGC 4151 performed by the Hopkins Ultraviolet Telescope during the Astro-2 mission. We show how the response of the Lyman continuum optical depth to variations…

Astrophysics · Physics 2007-05-23 J. H. Krolik , G. A. Kriss

We present the results of an intensive ground-based spectrophotometric monitoring campaign of the Seyfert galaxy NGC~4151 for a period of over two months, with a typical temporal resolution of one day. Light curves for four optical…

Astrophysics · Physics 2009-10-28 S. Kaspi et al

We disentangle X-ray disk reflection from complex line-of-sight absorption in the nearby Seyfert NGC 4151, using a suite of Suzaku, NuSTAR, and XMM-Newton observations. Extending upon earlier published work, we pursue a physically motivated…

High Energy Astrophysical Phenomena · Physics 2017-07-12 T. Beuchert , A. G. Markowitz , T. Dauser , J. A. García , M. L. Keck , J. Wilms , M. Kadler , L. W. Brenneman , A. A. Zdziarski

NGC 4151 is the brightest Seyfert 1 nucleus in X-rays. It was the first object to show short time delays in the Fe K band, which were attributed to relativistic reverberation, providing a new tool for probing regions at the black hole…

High Energy Astrophysical Phenomena · Physics 2019-10-16 Abderahmen Zoghbi , Jon Miller , Ed Cackett

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$_H$…

Astrophysics · Physics 2009-11-06 G. Risaliti , M. Elvis , F. Nicastro

On 9-11 May 1998, the highly-variable, low luminosity Seyfert 1 galaxy NGC4051 was observed in an unusual low flux state by BeppoSAX (Guainazzi et al. 1998) RXTE and EUVE. We present fits of the 4-15 keV RXTE spectrum and BeppoSAX MECS…

Astrophysics · Physics 2009-10-31 P. Uttley , I. M. McHardy , I. E. Papadakis , M. Guainazzi , A. Fruscione

We present a detailed analysis of the complex soft X-ray spectrum of NGC 4151 measured by the RGS instruments aboard XMM-Newton. The XMM-Newton RGS spectra demonstrate that the soft X-ray emission is extremely rich in X-ray emission lines…

Astrophysics · Physics 2009-11-10 N. J. Schurch , R. S. Warwick , R. E. Griffiths , S. M. Kahn

In this paper we present the analysis of two broad band (0.1-150 keV) BeppoSAX observations of the Seyfert 1 galaxy NGC 3516. The two observations were taken 4 months apart, on 1996 November 8 and 1997 March 12 respectively. We report a…

The Seyfert 1 galaxy NGC 5548 was observed for a week by Chandra using both the HETGS and LETGS spectrometers. In this paper we study the time variability of the continuum radiation. During our observation, the source showed a gradual…

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 report on soft X-ray observations of the Seyfert 1 galaxy MCG-6-30-15 with the Low and Medium Energy Concentrator Spectrometers on board BeppoSAX. The time averaged 0.1-4 keV spectrum shows evidence for a complex warm absorber. K-edges…

Astrophysics · Physics 2008-02-03 Astrid Orr , S. Molendi , F. Fiore , P. Grandi , A. N. Parmar , Alan Owens

We present a new X-ray analysis of the dwarf Seyfert galaxy NGC 4395, based on two archival XMM-Newton and Suzaku observations. This source is well known for a series of remarkable properties: one of the smallest estimated black hole masses…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Emanuele Nardini , Guido Risaliti

We present the results of the Suzaku observation of the Seyfert 2 galaxy NGC 4507. This source is one of the X-ray brightest Compton-thin Seyfert 2s and a candidate for a variable absorber. Suzaku caught NGC 4507 in a highly absorbed state…

High Energy Astrophysical Phenomena · Physics 2015-06-11 V. Braito , L. Ballo , J. N. Reeves , A. Ptak , G. Risaliti , T. J. Turner

During an extensive multiwavelength campaign that we performed in 2013-14 the prototypical Seyfert 1 galaxy NGC 5548 has been found in an unusual condition of heavy and persistent obscuration. The newly discovered "obscurer" absorbs most of…

This paper combines data from the three preceding papers in order to analyze the multi-waveband variability and spectral energy distribution of the Seyfert~1 galaxy NGC~4151 during the December 1993 monitoring campaign. The source, which…

Astrophysics · Physics 2009-10-28 R. A. Edelson et al

We report on 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, although the X-ray and…

Astrophysics · Physics 2009-10-31 B. M. Peterson , I. M. McHardy , B. J. Wilkes

An XMM-Newton observation of the luminous Seyfert 1 galaxy 1H 0419-577 in September 2002, when the source was in an extreme low-flux state, found a very hard X-ray spectrum at 1-10 keV with a strong soft excess below ~1 keV. Comparison with…

Astrophysics · Physics 2009-11-10 K. A. Pounds , J. N. Reeves , K. L. Page , P. T. O'Brien