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Related papers: Variable Intrinsic Absorption in Mrk 279

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We present a new method to model a HST/COS spectrum, aimed to analyze intrinsic UV absorption from the outflow of Mrk 290, a Seyfert I galaxy. We use newly updated XSTAR to generate photoionization models for the intrinsic absorption from…

Astrophysics of Galaxies · Physics 2015-06-23 S. N. Zhang , L. Ji , T. R. Kallman , Y. S. Yao , C. S. Froning , Q. S. Gu , G. A. Kriss

The Seyfert Galaxy Mrk 335 is known for its frequent changes of flux and spectral shape in the X-ray band occurred during recent years. These variations may be explained by the onset of a wind that previous, non-contemporaneous…

We propose a simple spectral model for the Seyfert 1 Galaxy MCG-6-30-15 that can explain most of the 1 - 40 keV spectral variation by change of the partial covering fraction, similar to the one proposed by Miller et al. (2008). Our spectral…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Takehiro Miyakawa , Ken Ebisawa , Hajime Inoue

We report results from a 2003 FUSE observation, and reanalysis of a 1996 HST observation of the unusual X-ray transient Narrow-line Seyfert 1 galaxy WPVS 007. The HST FOS spectrum revealed mini-BALs with V_max ~ 900 km s^-1 and FWHM ~ 550…

Cosmology and Nongalactic Astrophysics · Physics 2009-07-24 Karen M. Leighly , Fred Hamann , Darrin A. Casebeer , Dirk Grupe

We have examined the physical conditions in intrinsic UV-absorbing gas in the Seyfert galaxy NGC 4151, using echelle spectra obtained with the Space Telescope Imaging Spectrograph (STIS). We confirm the presence of the kinematic components…

We present the Chandra-LETGS analysis of Mrk 279, a bright Seyfert 1 galaxy. The spectrum shows a variety of features arising from different physical environments in the vicinity of the black hole. We detect three absorption components,…

Astrophysics · Physics 2009-11-10 E. Costantini , J. S. Kaastra , K. C. Steenbrugge , N. Arav , J. R. Gabel , G. Kriss

We present a study of the intrinsic UV absorption and emission lines in an historically low-state spectrum of the Seyfert 1 galaxy NGC 5548, which we obtained in 2004 February at high spatial and spectral resolution with the Space Telescope…

Astrophysics of Galaxies · Physics 2011-02-11 D. M. Crenshaw , S. B. Kraemer , H. R. Schmitt , J. S. Kaastra , N. Arav , J. R. Gabel , K. T. Korista

We present the discovery of an outflowing ionized wind in the Seyfert 1 Galaxy Mrk 335. Despite having been extensively observed by most of the largest X-ray observatories in the last decade, this bright source was not known to host warm…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 A. L. Longinotti , Y. Krongold , G. Kriss , J. Ely , L. Gallo , D. Grupe , S. Komossa , S. Mathur , A. Pradhan

We present medium resolution (R~20,000) HST/COS ultraviolet spectra covering 1155-1760 A of the Seyfert 1 Mrk 509 obtained simultaneously with a Chandra/LETGS spectrum as part of a multiwavelength campaign in 2009 that included observations…

We present new XMM-Newton observations of the intriguing warm absorber in I Zwicky 1. This luminous and nearby narrow-line Seyfert 1 galaxy shows ionized absorption by two components of outflowing gas; a low and a high-ionization phase with…

Astrophysics of Galaxies · Physics 2018-08-01 C. V. Silva , E. Costantini , M. Giustini , G. A. Kriss , W. N. Brandt , L. C. Gallo , D. R. Wilkins

We present the results of the analysis of the X-ray spectrum of the Seyfert 2 Mrk 348, observed by Suzaku and XMM-Newton. The overall spectrum of Mrk 348 can be described by a primary power law continuum seen through three layers of…

Astrophysics of Galaxies · Physics 2013-12-10 E. Marchese , V. Braito , J. N Reeves , R. Della Ceca , A. Caccianiga , A. Markowitz , G. Risaliti , P. Severgnini , T. J. Turner

The absorption lines in the soft X-ray spectrum of MCG--6-30-15 are studied using the Reflection Grating Spectrometer data from the 2001 XMM-Newton 320 ks observation. A line search of the full time-averaged spectrum reveals 51 absorption…

Astrophysics · Physics 2009-09-17 A. K. Turner , A. C. Fabian , J. C. Lee , S. Vaughan

To elucidate the location, physical conditions, mass outflow rate, and kinetic luminosity of the outflow from the active nucleus of the Seyfert 1 galaxy Mrk 509 we used coordinated ultraviolet and X-ray spectral observations in 2012 to…

There is growing evidence for the presence of blueshifted Fe K absorption lines in a number of radio-quiet AGNs and QSOs. These may be fundamental to probe flow dynamics near supermassive black holes. Here we aim at verifying and better…

High Energy Astrophysical Phenomena · Physics 2015-05-13 M. Cappi , F. Tombesi , S. Bianchi , M. Dadina , M. Giustini , G. Malaguti , L. Maraschi , G. G. C. Palumbo , P. O. Petrucci , G. Ponti , C. Vignali , T. Yaqoob

In about half of Seyfert galaxies, the X-ray emission is absorbed by an optically thin, ionized medium, the so-called "Warm Absorber", whose origin and location is still a matter of debate. The aims of this paper is to put more constraints…

We observed Mrk 509 during the fall of 2009 during a multiwavelength campaign using XMM-Newton, Chandra, HST/COS, SWIFT, and Integral. The 600-ks XMM/RGS spectrum finds two kinematic components and a discrete distribution of ionized…

The Seyfert 1 galaxy Mrk841 was observed five times between 2001 and 2005 by the XMM-Newton X-ray observatory. The source is well known for showing spectral complexity in the variable iron line and in the soft X-ray excess. This paper…

High Energy Astrophysical Phenomena · Physics 2015-05-14 A. L. Longinotti , E. Costantini , P. O. Petrucci , C. Boisson , M. Mouchet , M. Santos-Lleo , G. Matt , G. Ponti , A. C. Goncalves

We present observations of the UV absorption lines in the Seyfert 1 galaxy NGC 3783, obtained with the medium resolution echelle gratings of the Space Telescope Imaging Spectrograph(STIS) on the Hubble Space Telescope (HST). The spectra…

Astrophysics · Physics 2009-11-06 S. B. Kraemer , D. M. Crenshaw , J. R. Gabel

Mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the 2.5-11.7 micron spectrum. Contemporaneous optical photometric and…