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相关论文: High resolution X-ray spectroscopy and imaging of …

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We present results from spectral analysis of ASCA data on the NLS1 Mrk 507. This galaxy was found to have an exceptionally flat ROSAT spectrum among the NLS1s. The ASCA spectrum however shows a clear absorption feature in the energy band…

天体物理学 · 物理学 2009-10-30 K. Iwasawa , W. N. Brandt , A. C. Fabian

We present results of a high-resolution soft X-ray (0.2-2 keV) spectroscopic study of a sample of 69 nearby obscured Active Galactic Nuclei (AGN) observed with the Reflection Grating Spectrometer (RGS) on board XMM-Newton. This is the…

天体物理学 · 物理学 2008-11-26 Matteo Guainazzi , Stefano Bianchi

We have used non-simultaneous Ginga, ASCA and ROSAT observations to investigate the complex X-ray spectrum of the Seyfert 2 galaxy Mrk 3. We find that the composite spectrum can be well described in terms of a heavily cut-off hard X-ray…

天体物理学 · 物理学 2009-10-30 R. G. Griffiths , R. S. Warwick , I. Georgantopoulos , C. Done , D. A. Smith

We study the prototypical Seyfert 2 galaxy, Markarian 3, based on imaging and high-resolution spectroscopy observations taken by the Chandra X-ray Observatory. We construct a deconvolved X-ray image, which reveals the S-shaped morphology of…

高能天体物理现象 · 物理学 2017-10-18 Akos Bogdan , Ralph P. Kraft , Daniel A. Evans , Felipe Andrade-Santos , William R. Forman

We performed a detailed analysis of the Chandra and HST images of the Seyfert 2 galaxy, NGC7582. The dust lane, as mapped by the HST NIR and optical images, strongly influences the morphology of the soft X-ray emission, being spatially…

天体物理学 · 物理学 2008-11-26 Stefano Bianchi , Marco Chiaberge , Enrico Piconcelli , Matteo Guainazzi

We present and discuss Chandra and XMM-Newton observations of the Seyfert 2 galaxy and Compton-thick absorbed source, Tololo~0109-383. The hard X-ray emission (i.e. above $\sim$2 keV), is dominated by a spatially unresolved reflection…

天体物理学 · 物理学 2009-09-17 G. Matt , S. Bianchi , M. Guainazzi , W. N. Brandt , A. C. Fabian , K. Iwasawa , G. C. Perola

We present the soft X-ray spectrum of the LINER galaxy M81 from a long observation with the XMM-Newton RGS. As well as continuum emission from the active nucleus, the spectrum shows emission lines from multi temperature collisionally…

天体物理学 · 物理学 2007-05-23 M. J. Page , A. A. Breeveld , R. Soria , K. Wu

We present an analysis of the XMM-Newton observation of luminous infrared merging galaxies Arp 302 and a joint re-analysis of its Chandra observation. In particular, we focus on the more significant X-ray emitter of the pair, Arp 302N.…

高能天体物理现象 · 物理学 2024-01-09 Jiachen Jiang , William Baker , Andrew Young , Luigi Gallo

We present HST/WFPC2 images, in narrow-band filters containing the [OIII] lambda5007 and Halpha+[NII] emission-lines and their adjacent continua, of a sample of seven Seyfert 2 galaxies selected on the basis of possessing either extended…

天体物理学 · 物理学 2009-10-30 Heino Falcke , Andrew S. Wilson , Chris Simpson

We present optical SuperNova Integral Field Spectrograph (SNIFS) integral field spectroscopy, Hubble Space Telescope optical imaging, Chandra X-ray imaging, and Very Large Array radio interferometry of the merging galaxy 2MASX…

We present a detailed imaging analysis of 260 ks of sub-arcsecond resolution Chandra Advanced CCD Imaging Spectrometer (ACIS-S) observations of the nearby Seyfert 2 galaxy NGC 5728. Our study focuses on the bright and diffuse soft X-ray…

星系天体物理 · 物理学 2024-11-01 Anna Trindade Falcao , G. Fabbiano , M. Elvis , A. Paggi , W. P. Maksym

We report on a 100 ks Suzaku observation of the bright, nearby (z=0.008486) Seyfert 1.9 galaxy MCG -5-23-16. The broad-band (0.4-100 keV) X-ray spectrum allows us to determine the nature of the high energy emission with little ambiguity.…

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

We present the Chandra imaging and spectral analysis of NGC 4968, a nearby (z = 0.00986) Seyfert 2 galaxy. We discover extended ($\sim$1 kpc) X-ray emission in the soft band (0.5 - 2 keV) that is neither coincident with the narrow line…

We report near-infrared spectroscopic data for the Seyfert 2 galaxy Mrk 78, taken with the LIRIS near-infrared camera/spectrometer at the William Herschel Telescope (WHT). The long-slit spectra clearly show extended emission. The resolution…

We consider the properties of soft X-ray emission lines in the reprocessed emission from a photoionized accretion disc. Observations of these lines will be important in determining the ionization state and metallicity of the innermost…

天体物理学 · 物理学 2009-09-17 D. R. Ballantyne , R. R. Ross , A. C. Fabian

The X-ray spectra of some active galactic nuclei (AGN) show a soft X-ray excess, emission in excess to the extrapolated primary X-ray continuum below 2 keV. Recent studies have shown that this soft excess can be described well as…

高能天体物理现象 · 物理学 2022-10-26 S. Chalise , A. M. Lohfink , J. Chauhan , T. D. Russell , D. J. K. Buisson , L. Mallick

We measure the metal abundance ratios in the X-ray photoionized gas located near the narrow line region of a sample of Seyfert 2 AGN. The high-resolution X-ray spectra observed with the Chandra high- and low-energy transmission grating…

天体物理学 · 物理学 2017-08-23 Mario A. Jimenez-Garate , Toan Khu

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

A number of radio galaxies has been detected by Fermi/LAT in the gamma-ray domain. In some cases, like Cen A and M 87, these objects have been seen even in the TeV range by Cherenkov telescopes. Whereas the gamma-ray emission is likely to…

高能天体物理现象 · 物理学 2013-02-20 V. Beckmann , S. de Jong , F. Mattana , D. Saez , S. Soldi