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相关论文: A Deep ROSAT HRI Observation of NGC 1313

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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 report the results of a deep spatial, spectral, and timing analysis of ROSAT HRI and PSPC observations of the edge-on starburst galaxy NGC 253. In this first paper, point-like X-ray sources detected within the galaxy and in the field are…

天体物理学 · 物理学 2007-05-23 A. Vogler , W. Pietsch

We present the preliminary results of a deep (167 ks) ROSAT HRI observation of the cD galaxy NGC1399 in the Fornax cluster. We find, in agreement with previous observations, an extended (41 Kpc adopting a distance of 19 Mpc) gaseous halo…

天体物理学 · 物理学 2007-05-23 M. Paolillo , G. Fabbiano , G. Peres , D. -W. Kim

We use the extensive public archive of ROSAT High Resolution Imager (HRI) observations to carry out a statistical investigation of the X-ray properties of nearby galaxies. Specifically we focus on the sample of 486 bright (B_T < 12.5)…

天体物理学 · 物理学 2009-10-31 T. P. Roberts , R. S. Warwick

We present an analysis of recent XMM-Newton and HST archive data of the ultraluminous X-ray source NGC 1313 X-2. Quasi-simultaneous observations taken with XMM-Newton, HST and VLT allow us to study both the X-ray light curve and its…

天体物理学 · 物理学 2015-06-24 P. Mucciarelli , L. Zampieri , A. Treves , R. Turolla , R. Falomo

The ROSAT Deep Survey in the Lockman Hole is the most sensitive X-ray survey performed to date, encompassing an exposure time of 200 ksec with the PSPC and 1.2 Msec with the HRI. The source counts reach a density of ~1000/deg2 at a limiting…

天体物理学 · 物理学 2007-05-23 G. Hasinger , I. Lehmann , R. Giacconi , M. Schmidt , J. Truemper , G. Zamorani

We present an XMM-Newton observation of the massive edge-on Sb galaxy NGC 2613. We discover that this galaxy contains a deeply embedded active nucleus with a 0.3-10 keV luminosity of 3.3x10^40 erg/s and a line-of-sight absorption column of…

天体物理学 · 物理学 2009-11-11 Zhiyuan Li , Q. Daniel Wang , Judith A. Irwin , Tara Chaves

The emission-line dwarf galaxy NGC 3413 is known to host a bright X-ray source near its optical center. The 0.3-10 keV luminosity of this source is estimated to be approximately 10$^{39}$ erg$s^{-1}$ potentially qualifying it as an…

高能天体物理现象 · 物理学 2018-10-17 E. Sonbas , K. S. Dhuga , E. Göğüş

All 543 pointed observations of the ROSAT High Resolution Imager (HRI) with exposure times higher than 50 sec in a field of 10 deg x 10 deg covering the Large Magellanic Cloud (LMC) were analyzed. A catalogue was produced containing 397…

天体物理学 · 物理学 2009-10-31 Manami Sasaki , Frank Haberl , Wolfgang Pietsch

We report on 40 kiloseconds of ROSAT HRI observations of the globular cluster M92 (NGC 6341) and 20 kiloseconds of observations of the globular cluster M13 (NGC 6205). We find that the low-luminosity (10^{32.5} erg/sec at 7.5 kpc) source…

天体物理学 · 物理学 2015-06-24 D. Fox , W. Lewin , B. Margon , J. van Paradijs , F. Verbunt

We discuss ROSAT HRI X-ray observations of 33 very nearby galaxies, sensitive to X-ray sources down to a luminosity of approximately 10^38 erg/s. The galaxies are selected from a complete, volume limited sample of 46 galaxies with d<7 Mpc…

天体物理学 · 物理学 2009-10-31 P. Lira , A. Lawrence , R. A. Johnson

A ROSAT HRI X-ray image was obtained of the open globular cluster NGC 288, which is located near the South Galactic Pole. This is the first deep X-ray image of this system. We detect a Low Luminosity Globular Cluster X-ray source (LLGCX)…

The E3 giant elliptical galaxy NGC5018 was observed with the Chandra X-ray Observatory on 14 April 2001. Results of analysis of these X-ray data as well as of complementary optical, infrared, and radio data are reported. Seven X-ray point…

天体物理学 · 物理学 2009-11-10 Kajal K. Ghosh , Douglas A. Swartz , Allyn F. Tennant , Kinwah Wu , Lakshmi Saripalli

We update the light curves from the X-ray, optical, and radio bandpasses which we have assembled over the past decade, and present two observations in the ultraviolet using the Hubble Space Telescope Faint Object Spectrograph. The HRI X-ray…

天体物理学 · 物理学 2009-10-31 Eric M. Schlegel , Stuart Ryder , L. Staveley-Smith , R. Petre , E. Colbert , M. Dopita , D. Campbell-Wilson

The nearby barred spiral galaxy NGC 1672 is thought to have a weak Seyfert nucleus in addition to its strong starburst activity. Observations with the PSPC and HRI instruments on board the ROSAT X-ray satellite show that three X-ray sources…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , J. P. Halpern , K. Iwasawa

We have observed NGC 1316 (Fornax A) with the ROSAT HRI. In this paper, we present the results of these observations and we complement them with the spectral analysis of the archival PSPC data. The spectral properties suggest the presence…

天体物理学 · 物理学 2009-10-30 Dong-Woo Kim , Giuseppina Fabbiano , Glen Mackie

We report the results of XMM-Newton observations for an especially luminous supersoft X-ray source (SSS) with bolometric luminosity of 10^39 erg/s in the spiral galaxy NGC 300. The source was detected as a SSS in 1992 and disappeared in…

天体物理学 · 物理学 2009-11-07 A. K. H. Kong , R. Di Stefano

We report the detection of luminous extended X-ray emission in NGC 6240 on the basis of ROSAT HRI observations of this ultraluminous IR galaxy. The spatial structure and temporal behavior of the X-ray source were analyzed. We find that >=…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa , Hartmut Schulz , Jochen Greiner

The Type IIn supernova (SN) 1978K in the nearby galaxy NGC 1313 has remained bright in multiwavelengths for more than $\sim 25$ yr. The archival data of SN 1978K collected with ROSAT, ASCA, XMM-Newton, and Chandra from 1990 to 2006 show no…

高能天体物理现象 · 物理学 2017-04-20 Hai-Hui Zhao , Shan-Shan Weng , C. -Y. Ng

We report on pointed X-ray observations of IC 10, NGC 147 and NGC 185 made with the ROSAT High Resolution Imager (HRI). These are three Local Group galaxies that have never been previously studied in detail in the X-ray regime. IC 10 is the…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , M. J. Ward , A. C. Fabian , P. W. Hodge
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