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Related papers: Steep Spectrum Seyfert Galaxies

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Narrow Line Seyfert 1 galaxies (NLS1) are very interesting objects which display peculiar properties when compared to their broad line analogues (BLS1). Although well studied in many wavebands, their behaviour at >10 keV is poorly studied…

The results of spectropolarimetry surveys of obscured AGNs are reviewed, paying special attention to their implications for the existence of two populations of type 2 Seyfert galaxies -- hidden Seyfert 1s and "true" Seyfert 2s. In this…

Astrophysics · Physics 2007-05-23 Edward C. Moran

The discovery of gamma-ray emission from 5 radio-loud narrow-line Seyfert 1 galaxies revealed the presence of a possible emerging third class of AGNs with relativistic jets, in addition to blazars and radio galaxies. The existence of…

High Energy Astrophysical Phenomena · Physics 2019-08-13 F. D'Ammando , M. Orienti , J. Finke , J. Larsson , M. Giroletti

We report on simultaneous ASCA and ROSAT observations of the Seyfert galaxy NGC5548 made during the ASCA Performance Verification phase. Spectral features due to a warm absorber and reflection are clearly seen in the X-ray spectra. We find…

Astrophysics · Physics 2009-10-31 K. Iwasawa , A. C. Fabian , K. Nandra

The mass of the central black hole in Seyfert galaxies and QSOs can be determined from the broad emission lines and the reverberation method. Using the measured black hole mass and the bolometric or ionizing luminosity, the accretion rate…

Astrophysics · Physics 2009-10-31 Youjun Lu , Qingjuan Yu

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 define a new sample of 96 low-redshift (z<0.1), soft X-ray selected Seyferts from the catalog of the Einstein Slew Survey (Elvis etal. 1992, Plummer et al. 1994). We probe the geometry and column depth of obscuring material in the…

Astrophysics · Physics 2009-10-30 Robert Simcoe , K. K. McLeod , Jonathan Schachter , Martin Elvis

We discuss the properties of the Seyfert 1.5 galaxy LB 1727, also known as 1H 0419-577, from X-ray observations obtained by ASCA and ROSAT along with optical observations from earlier epochs. ASCA shows only modest (< 20%) variations in…

An XMM-Newton observation of the luminous Seyfert galaxy PG1211+143 in 2001 revealed the first clear evidence for a highly ionised high speed wind (in a non-BAL AGN), with a velocity of v~0.09c based on the identification of blue-shifted…

High Energy Astrophysical Phenomena · Physics 2015-06-17 K. A. Pounds

X-ray binaries are known to show state transitions related to accretion rate changes which are often accompanied with dramatic changes in the jet emission. However, it is not clear whether this characteristics of stellar-mass black hole…

Astrophysics of Galaxies · Physics 2023-04-21 K. É. Gabányi , K. Smith , S. Frey , Z. Paragi , T. An , A. Moór

Blueshifted absorption lines in the X-ray spectra of AGN show that ultra-fast outflows with typical velocities $v \sim 0.1c$ are a common feature of these luminous objects. Such powerful AGN winds offer an explanation of the observed…

High Energy Astrophysical Phenomena · Physics 2018-09-12 Ken Pounds , Chris Nixon , Andrew Lobban , Andrew King

We probed the relation between properties of Seyfert nuclei and morphology of their host galaxies. We selected Seyfert galaxies from the Sloan Digital Sky Survey with redshifts less 0.2 identified by the V\'{e}ron Catalog (13th). We used…

Astrophysics of Galaxies · Physics 2017-12-20 Yen-Chen Chen , Chorng-Yuan Hwang

The Seyfert galaxy NGC 6814 is a highly variable X-ray source despite the fact that it has recently been shown not to be the source of periodic variability. The 1.5 year monitoring by ROSAT has revealed a long term downward trend of the…

Astrophysics · Physics 2007-05-23 Michael Koenig , Susanne Friedrich , Ruediger Staubert , Jens Timmer

We examine the XMM X-ray spectrum of the LINER-AGN NGC 7213, which is best fit with a power law, K-alpha emission lines from Fe I, Fe XXV and Fe XXVI and a soft X-ray collisionally ionised thermal plasma with kT=0.18 +0.03/-0.01 keV. We…

Astrophysics · Physics 2009-11-10 R. L. C. Starling , M. J. Page , G. Branduardi-Raymont , A. A. Breeveld , R. Soria , K. Wu

A ROSAT observation of the narrow-line Fe II QSO PHL 1092 shows rapid variability that requires an efficiency of at least 0.13, exceeding the theoretical maximum for an accretion disk around a non-rotating black hole. Plausible explanations…

Astrophysics · Physics 2009-10-28 Karl Forster , Jules P. Halpern

We examine the accretion properties in a sample of 42 hard (3-60keV) X-ray selected nearby broad-line AGNs. The energy range in the sample is harder than that usually used in the similar previous studies. These AGNs are mainly complied from…

Astrophysics · Physics 2011-02-19 J. Wang , Y. F. Mao , J. Y. Wei

We study the utility of broad-band colours in the SkyMapper Southern Survey for selecting Seyfert galaxies at low luminosity. We find that the $u-v$ index, built from the ultraviolet $u$ and violet $v$ filters, separates normal galaxies,…

Astrophysics of Galaxies · Physics 2020-10-21 Christian Wolf , Jacob Golding , Wei Jeat Hon , Christopher A. Onken

We present a study of the X-ray properties of a volume-limited sample of optically selected emission-line galaxies. The sample is derived from a correlation between the KPNO International Spectroscopic Survey (KISS), an H-alpha-selected…

Astrophysics · Physics 2009-11-07 Samantha L. Stevenson , John J. Salzer , Vicki L. Sarajedini , Edward C. Moran

We present a comprehensive analysis of the timing and spectral properties of NGC 7314, a Seyfert 1.9 galaxy, using X-ray observations from {\it XMM-Newton}, {\it NuSTAR}, and {\it RXTE}/PCA. The timing analysis reveals significant…

High Energy Astrophysical Phenomena · Physics 2024-10-03 Debjit Chatterjee , Arghajit Jana , A. Mangalam , Hsiang-Kuang Chang

We discuss the hard X-ray properties of the Seyfert galaxy Ton S 180, based upon the analysis of ASCA data. We find the X-ray flux varied by a factor ~2 on a time scale of a few thousand seconds. The source showed significantly higher…

Astrophysics · Physics 2009-10-30 T. J. Turner , I. M. George , K. Nandra
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