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Related papers: Variable Iron K-alpha Lines in Seyfert 1 Galaxies

200 papers

We report the detection of a narrow Fe-K emission line in the Seyfert 1 galaxy NGC 5548 with the Chandra High-Energy Transmission Gratings. In the galaxy frame we measure a center energy of 6.40 \pm 0.03 keV, a FWHM of 4515 (+3525,-2645)…

Astrophysics · Physics 2009-10-31 T. Yaqoob , I. M. George , K. Nandra , T. J. Turner , P. J. Serlemitsos , R. F. Mushotzky

We present a detailed re-analysis of the two {\it ASCA} Performance Verification observations of the nearby Seyfert 1 galaxy MCG-6-30-15. Confirming the results of Fabian et al. (1994), we find definite evidence for the {\sc O\,vii} and…

Astrophysics · Physics 2015-06-24 C. S. Reynolds , A. C. Fabian , K. Nandra , H. Inoue , H. Kunieda , K. Iwasawa

We present an analysis of the relativistic iron K-alpha line in the Seyfert 1 galaxy NGC 3516, based on a continuous, five-day ASCA observation. The broad profile which has been found in several other AGN is confirmed in NGC 3516 with…

Astrophysics · Physics 2009-10-31 K. Nandra , I. M. George , R. F. Mushotzky , T. J. Turner , T. Yaqoob

We present an analysis of the long RXTE observation of the Seyfert~1 galaxy MCG-6-30-15, taken in July 1997. Our results show that the behaviour is complicated. We find clear evidence from colour ratios and direct spectral fitting that…

Astrophysics · Physics 2009-09-17 J. C. Lee , A. C. Fabian , C. S. Reynolds , W. N. Brandt , K. Iwasawa

We present an analysis of the X-ray variability properties of the NLS1 galaxy Ton S180, based upon a 12-day continuous ASCA observation. We observe flux variations of a factor of 3.5 in the 0.7-1.3 keV band and 3.9 in the 2-10 keV…

Astrophysics · Physics 2008-11-26 P. Romano , T. J. Turner , S. Mathur , I. M. George

Recent XMM-Newton observations have measured the hard (2.5-12 keV) X-ray spectrum of the well-known Seyfert galaxy NGC 4151 with a signal-to-noise unprecedented for this source. We find that a spectral model, developed to fit previous…

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

We present simultaneous observations by EUVE, ASCA, and RXTE of the type~1 Seyfert galaxy NGC 5548. These data indicate that variations in the EUV emission (at $\sim 0.2 $keV) appear to lead similar modulations in higher energy ($\ga 1…

We report on the results from a large observational campaign on the bare Seyfert galaxy Ark 120, jointly carried out in 2014 with XMM-Newton, Chandra, and NuSTAR. The fortunate line of sight to this source, devoid of any significant…

High Energy Astrophysical Phenomena · Physics 2016-11-23 E. Nardini , D. Porquet , J. N. Reeves , V. Braito , A. Lobban , G. Matt

This paper presents a comprehensive study of the X-ray properties of low-ionization nuclear emission-line regions (LINERs) and low-luminosity Seyfert galaxies based on observations obtained with ASCA. We analyzed data of 53 observations of…

Astrophysics · Physics 2009-11-07 Yuichi Terashima , Naoko Iyomoto , Luis C. Ho , Andrew F. Ptak

This paper presents a quantification of the X-ray variability amplitude for 79 ASCA observations of 36 Seyfert 1 galaxies. We find that consideration of sources with the narrowest permitted lines in the optical band introduces scatter into…

Astrophysics · Physics 2009-10-31 T. J. Turner , I. M. George , K. Nandra , D. Turcan

We present the results of an ASCA observation of the LINER NGC 4579. A point-like X-ray source is detected at the nucleus with a 2-10 keV luminosity of 1.5x10^41 ergs/s assuming a distance of 16.8 Mpc. The X-ray spectrum is represented by a…

A 2012 Suzaku observation of the Seyfert 1.5 galaxy Markarian 530 was analysed and found to exhibit two distinct modes of variability, which were found to be independent from one another. Firstly, the spectrum undergoes a smooth transition…

High Energy Astrophysical Phenomena · Physics 2018-06-06 H. J. S. Ehler , A. G. Gonzalez , L. C. Gallo

We report on a 50 ks observation of the bright Seyfert 1 galaxy MCG--6-30-15 with the Rossi X-ray Timing Explorer. The data clearly show the broad fluorescent iron line (equivalent width ~ 250 eV), and the Compton reflection continuum at…

Astrophysics · Physics 2009-10-30 J. C. Lee , A. C. Fabian , C. S. Reynolds , K. Iwasawa , W. N. Brandt

We present an analysis of the X-ray spectra of a sample of 37 observations of 26 Seyfert galaxies observed by XMM-Newton in order to characterize their iron K emission. All objects show evidence for iron line emission in the 6-7 keV band. A…

Astrophysics · Physics 2009-11-13 K. Nandra , P. M. O'Neill , I. M. George , J. N. Reeves

Preliminary results from an X-ray spectral study of Seyfert 1 galaxies with ASCA and RXTE are presented. From an analysis of X-ray reprocessing features of Compton reflection and Fe K-alpha fluorescence, it is found that iron line strength…

Astrophysics · Physics 2009-10-31 K. A. Weaver

The unprecedented sensitivity of current X-ray telescopes allows for the first time to address the issue of the Fe K line complex variability patterns in bright, nearby AGNs. We examine XMM-Newton observations of the brightest sources of…

High Energy Astrophysical Phenomena · Physics 2015-05-13 B. De Marco , K. Iwasawa , M. Cappi , M. Dadina , F. Tombesi , G. Ponti , A. Celotti , G. Miniutti

The bright, soft X-ray spectrum Seyfert 1 galaxies Ark 564 and Ton S180 were monitored for 35 days and 12 days with ASCA and RXTE (and EUVE for Ton S180). The short time scale (hours-days) variability patterns were very similar across…

We present the light curves obtained during an eight-year program of optical spectroscopic monitoring of nine Seyfert 1 galaxies: 3C 120, Akn 120, Mrk 79, Mrk 110, Mrk 335, Mrk 509, Mrk 590, Mrk 704, and Mrk 817. All objects show…

We present simultaneous ASCA and RXTE data on the bright Seyfert 1 galaxy IC4329a. The iron line is significantly broadened, but not to the extent expected from an accretion disk which extends down to the last stable orbit around a black…

Astrophysics · Physics 2009-10-31 C. Done , G. M. Madejski , P. T. Zycki

We present an analysis of five Suzaku observations of the bright Seyfert1 galaxy IC 4329A. The broad energy band and high signal-to-noise ratio of the data give new constraints on the iron K alpha line profile and its relationship with the…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Giulia Mantovani , Kirpal Nandra , Gabriele Ponti