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相关论文: The flat X-ray spectrum of the LINER NGC1052

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The first X-ray observation of the Seyfert 2 galaxy NGC5252 is reported. ASCA collected $\sim 4000$ photons/detector enough to perform an accurate spectral analysis of this source. The luminosity of NGC5252 is L$_{\rm X}$(0.7-10 keV)…

天体物理学 · 物理学 2009-10-28 M. cappi , T. Mihara , M. Matsuoka , W. Brinkmann , M. A. Prieto , G. G. C. Palumbo

We examine the 0.1 to 10.0 keV X-ray spectrum of the bright nuclear LINER galaxy NGC 1052, one of two elliptical galaxies known to contain a luminous H2O maser. The observed 2.0-10.0 keV spectrum is unusually flat (photon index Gamma~0.2)…

天体物理学 · 物理学 2009-10-31 K. A. Weaver , A. S. Wilson , C. Henkel , J. A. Braatz

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

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…

天体物理学 · 物理学 2009-11-07 Yuichi Terashima , Naoko Iyomoto , Luis C. Ho , Andrew F. Ptak

We present an investigation of the X-ray properties of 13 LINERs based on ROSAT all-sky survey and pointed PSPC and HRI observations. Several sources are studied for the first time in X-rays. The X-ray spectra are best described by a…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Hans Boehringer , John P. Huchra

I present ASCA observations of IRAS00317-2142, the most luminous (Lx~10^43 erg s-1 0.1-2 keV) of the 'composite' class of galaxies. This enigmatic class of objects presents narrow-emission line optical spectra classifying these galaxies as…

天体物理学 · 物理学 2009-10-31 I. Georgantopoulos

We report on the discovery of a narrow-emission-line object at z=0.672 detected in a deep ASCA survey. The object, AXJ0341.4-4453, has a flux in the 2--10keV band of 1.1+/-0.27 E-13 erg/s/cm**2, corresponding to a luminosity of 1.8E44 erg/s…

Optical spectropolarimetry of the nucleus of the LINER NGC 1052, obtained at the Keck Observatory, reveals a rise in polarization in the wings of the H-alpha line profile. The polarization vector of H-alpha is offset by 67 degrees from the…

天体物理学 · 物理学 2009-10-31 A. J. Barth , A. V. Filippenko , E. C. Moran

We present observations in the 0.1-100 keV spectral band of 8 Seyfert 2 galaxies, obtained by means of BeppoSAX. These sources were selected according to their [OIII] optical emission line flux, to avoid biases against obscuration on the pc…

天体物理学 · 物理学 2007-05-23 R. Maiolino , M. Salvati , L. Bassani , M. Dadina , R. Della Ceca , G. Matt , G. Risaliti , G. Zamorani

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

We present Chandra observations of the enigmatic galaxy IRAS00317-2142, which is classified as a star-forming galaxy on the basis of the ionization level of its emission lines. However, a weak broad H\alpha wing and a high X-ray luminosity…

天体物理学 · 物理学 2016-08-30 I. Georgantopoulos , A. Zezas , M. J. Ward

We analyze the 0.5-10 keV spectra of six Seyfert 2 galaxies observed with the X-ray satellite ASCA: Mrk 3, Mrk 348, Mrk 1210, Mrk 477, NGC 7212, and Was 49b. These galaxies were selected based on their possession of optical polarized broad…

天体物理学 · 物理学 2016-08-30 Hisamitsu Awaki , Shiro Ueno , Yoshiaki Taniguchi , Kimberly A. Weaver

We present an analysis of the 101 ks, 2007 Suzaku spectrum of the LINER galaxy NGC 1052. The 0.5-10 keV continuum is well-modeled by a power-law modified by Galactic and intrinsic absorption, and it exhibits a soft, thermal emission…

高能天体物理现象 · 物理学 2011-02-11 L. W. Brenneman , K. A. Weaver , M. Kadler , J. Tueller , A. Marscher , E. Ros , A. Zensus , Y. Y. Kovalev , M. Aller , H. Aller , J. Irwin , J. Kerp , S. Kaufmann

We present ROSAT HRI and ASCA observations of the well known ULIRG IRAS19254-7245 (the Superantennae). The object is not detected by ROSAT yielding a 3\sigma upper limit of L_x ~8x10^{41} erg/s in the 0.1-2 keV band. However, we obtain a…

天体物理学 · 物理学 2009-10-31 A. Pappa , I. Georgantopoulos , G. C. Stewart

We present a study of available Hubble Space Telescope (HST) spectroscopic and imaging observations of the low ionization nuclear emission line region (LINER) galaxy NGC 1052. The WFPC2 imagery clearly differentiates extended nebular Halpha…

天体物理学 · 物理学 2009-10-31 J. R. Gabel , F. C. Bruhweiler , D. M. Crenshaw , S. B. Kraemer , C. L. Miskey

We present ASCA GIS observations (total exposure 100-200 ksec) of three fields which form part of our deep ROSAT survey. We detect 26 sources down to a limiting flux (2-10 keV) of 5x10^{-14} erg cm-2 s-1. Sources down to this flux level…

Suzaku observed a nearby Seyfert 2 galaxy NGC4945, which hosts one of the brightest active galactic nuclei above 20 keV. Combining data from the X-ray CCD camera (XIS) and the Hard X-ray Detector (HXD), the AGN intrinsic nuclear emission…

The wide-band energy spectrum of NGC6240 over the range 0.5-200keV is investigated using the RXTE and ASCA data. The RXTE data provide the spectrum beyond the ASCA range (0.5-10 keV) with significant detection of signals up to 20keV and the…

天体物理学 · 物理学 2009-10-31 Yasushi Ikebe , Karen Leighly , Yasuo Tanaka , Takao Nakagawa , Yuichi Terashima , Stefanie Komossa

We have discovered a Narrow-Line Seyfert 1 (NLS1) galaxy and identified it with an ultrasoft X-ray source RX 215319-1514 detected with ROSAT. We present its X-ray and optical spectral characteristics. Its redshift is found to be…

天体物理学 · 物理学 2007-05-23 K. P. Singh , L. R. Jones

We present the first high-resolution, soft-X-ray spectrum of the prototypical Seyfert 2 galaxy, NGC 1068. This spectrum was obtained with the XMM-Newton Reflection Grating Spectrometer. Emission lines from H-like and He-like low-Z ions…

天体物理学 · 物理学 2009-11-07 A. Kinkhabwala , M. Sako , E. Behar , S. M. Kahn , F. Paerels , A. C. Brinkman , J. S. Kaastra , M. F. Gu , D. A. Liedahl
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