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相关论文: The soft X-ray/NLR connection: a single photoioniz…

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We present the soft X-ray spectrum of the LINER galaxy M81 derived from a long observation with the XMM RGS. The spectrum is dominated by continuum emission from the active nucleus, but also contains emission lines from Fe L, and H-like and…

天体物理学 · 物理学 2009-11-07 M. J. Page , A. A. Breeveld , R. Soria , K. Wu , G. Branduardi-Raymont , K. O. Mason , R. L. C. Starling , S. Zane

The nearby barred spiral galaxy NGC 1313 has been observed with the PSPC instr- ument on board the ROSAT X-ray satellite. Ten individual sources are found. Three sources (X-1, X-2 and X-3 [SN~1978K]) are very bright (~10^40 erg/s) and are…

天体物理学 · 物理学 2016-08-30 E. J. M. Colbert , R. Petre , E. M. Schlegel , S. D. Ryder

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…

天体物理学 · 物理学 2009-11-10 N. J. Schurch , R. S. Warwick , R. E. Griffiths , S. M. Kahn

We present a spectral analysis of the narrow-line Seyfert 1 galaxy I Zwicky 1, focusing on the characteristics of the ionised absorbers as observed with XMM-Newton in 2005. The soft X-ray spectrum shows absorption by two components of…

天体物理学 · 物理学 2008-11-26 E. Costantini , L. C. Gallo , W. N. Brandt , A. C. Fabian , Th. Boller

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…

天体物理学 · 物理学 2009-10-31 T. J. Turner , I. M. George , K. Nandra , D. Turcan

We present the results of the spatial and spectral analysis of the deep (~200 ksec) Chandra HETG observation of the changing look AGN NGC7582. During this observation NGC7582 was in a highly obscured state. Therefore, we considered also a…

高能天体物理现象 · 物理学 2017-04-19 Valentina Braito , James Reeves , Stefano Bianchi , Emanuele Nardini , Enrico Piconcelli

We present results from a ~55 ks long XMM-Newton observation of the obscured AGN, NGC 5643, performed in July 2009. A previous, shorter (about 10 ks) XMM-Newton observation in February 2003 had left two major issues open, the nature of the…

高能天体物理现象 · 物理学 2015-06-16 G. Matt , S. Bianchi , A. Marinucci , M. Guainazzi , K. Iwawasa , E. Jimenez Bailon

Ultra-soft narrow line Seyfert 1 (US-NLSy) are a poorly observed class of active galactic nuclei characterized by significant flux changes and an extreme soft X-ray excess. This peculiar spectral shape represents a golden opportunity to…

RS Cae is the third target in our series of XMM-Newton observations of soft X-ray-dominated polars. Our observational campaign aims to better understand and describe the multiwavelength data, the physical properties of the system…

太阳与恒星天体物理 · 物理学 2014-01-08 I. Traulsen , K. Reinsch , A. D. Schwope , R. Schwarz , F. M. Walter , V. Burwitz

XMM-Newton and Chandra/HETG spectra of the Compton-thin (NH 4x10^{23} cm^{-2}) Seyfert 2 galaxy, NGC 4507, are analyzed and discussed. The main results are: a) the soft X-ray emission is rich in emission lines; an (at least) two--zone…

天体物理学 · 物理学 2009-11-10 Giorgio Matt , Stefano Bianchi , Filippo D'Ammando , Andrea Martocchia

We use the full broad-band XMM-Newton EPIC data to examine the X-ray spectrum of the nearby Seyfert 2 galaxy NGC 1068, previously shown to be complex with the X-ray continuum being a sum of components reflected/scattered from cold (neutral)…

天体物理学 · 物理学 2009-11-11 K. Pounds , S. Vaughan

During the disk-mediated accretion phase, the high-resolution X-ray spectrum of the low-mass X-ray binary system EXO 0748-676 reveals a photoionized plasma which is orbiting the neutron star. Our observations with the Chandra High Energy…

天体物理学 · 物理学 2008-11-26 M. A. Jimenez-Garate , N. S. Schulz , H. L. Marshall

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…

高能天体物理现象 · 物理学 2015-06-17 K. A. Pounds

We present XMM-Newton observations of four low-redshift Seyfert galaxies selected to have low host luminosities (M_g>-20 mag) and small stellar velocity dispersions (sigma_star<45 km/s), which are among the smallest stellar velocity…

宇宙学与河外天体物理 · 物理学 2014-11-20 C. E. Thornton , A. J. Barth , L. C. Ho , J. E. Greene

We report results obtained from six XMM-Newton observations of the Seyfert galaxy 1H 0419-577. Here we show that the X-ray spectrum and variability are well described by a two-component model comprising a power law with constant spectral…

天体物理学 · 物理学 2009-09-17 A. C. Fabian , G. Miniutti , K. Iwasawa , R. R. Ross

We present a sample of twenty-one ROSAT bright active galactic nuclei (AGN), representing a range of spectral classes, and selected for follow-up snap-shot observations with XMM-Newton. The typical exposure was between 5-10 ks. The objects…

天体物理学 · 物理学 2009-11-13 L. C. Gallo , I. Lehmann , W. Pietsch , Th. Boller , W. Brinkmann , P. Friedrich , D. Grupe

The observed spatial and kinematic overlap between soft X-ray emission and the Narrow Line Region (NLR) in obscured Active Galactic Nuclei (AGN) yields compelling evidence that relatively low-density gas co-exists with higher density gas on…

高能天体物理现象 · 物理学 2019-02-20 Stefano Bianchi , Matteo Guainazzi , Ari Laor , Jonathan Stern , Ehud Behar

We present soft X-ray results from observations with the Chandra HETGS of the Seyfert I AGN NGC 4593 and Mrk 509. We discuss the photoionized outflows associated with Seyfert I AGN in terms of their absorption spectral signatures and…

天体物理学 · 物理学 2007-05-23 B. McKernan , T. Yaqoob

We report X-ray fluxes in the 2--10 keV band from LINERs (low-ionization nuclear emission-line regions) and low-luminosity Seyfert galaxies obtained with the ASCA satellite. Observed X-ray luminosities are in the range between 4e39 and 5e41…

天体物理学 · 物理学 2009-10-31 Yuichi Terashima , Luis C. Ho , Andrew F. Ptak

We present XMM-Newton/EPIC spectra for the Laor et al. sample of Palomar Green quasars. We find that a power-law provides a reasonable fit to the 2-5 keV region of the spectra. Excess soft X-ray emission below 2 keV is present for all…