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相关论文: ROSAT observation of GRS 1739-278

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For the first time X-ray bursts have been detected from a sky position consistent with the one of GRS 1741.9-2853, a GRANAT transient source located only ~10' from the Galactic Centre. A total of 3 bursts have been observed by the Wide…

天体物理学 · 物理学 2007-05-23 M. Cocchi , A. Bazzano , L. Natalucci , P. Ubertini , J. Heise , J. M. Muller , J. J. M. in 't Zand

We present quasi-simultaneous radio and X-ray observations of the black hole X-ray binary GRS 1739--278 of its 2015-2016 mini-outbursts, i.e. between 2015 June 10 and 2016 October 31, with the X-ray-to-radio time interval being less than…

高能天体物理现象 · 物理学 2020-03-11 Fu-Guo Xie , Zhen Yan , Zhongzu Wu

We present X-ray observations of the narrow line radio galaxy 1138-262 at z = 2.156 with the High Resolution Imager (HRI) on ROSAT. Observations at other wave-bands, and in particular extremely high values of Faraday rotation of the…

天体物理学 · 物理学 2015-06-24 C. L. Carilli , D. E. Harris , L. Pentericci , H. J. A. Rottgering , G. K. Miley , M. N. Bremer

We present a detailed spectral analysis of XMM-Newton and NuSTAR observations of the accreting transient black hole GRS 1739-278 during a very faint low hard state at ~0.02% of the Eddington luminosity (for a distance of 8.5 kpc and a mass…

We present the results of three ROSAT HRI observations of AGN expected to reside in clusters of galaxies. Although the exposures were truncated by the premature end of the ROSAT mission, valuable information could be achieved which greatly…

天体物理学 · 物理学 2007-05-23 M. Gliozzi , W. Brinkmann , S. A. Laurent-Muehleisen , L. O. Takalo , A. Sillanpaa

We report the first detection of a time-dependent, dust-scattered X-ray halo around a gamma-ray burst. GRB 031203 was observed by XMM-Newton starting six hours after the burst. The halo appeared as concentric ring-like structures centered…

The X-ray nova GRS1739-278 flared up near the Galactic center in the spring of 1996. Here we report on the discovery of a ~5-Hz quasi-periodic oscillations (QPO) in RXTE/PCA observations of GRS1739-278. The QPO were only present when the…

天体物理学 · 物理学 2015-06-24 K. N. Borozdin , S. P. Trudolyubov

We present a 10-year X-ray light curve and the spectra of a peculiar X-ray transient in the spiral galaxy M81. The source was below the detection limit of ROSAT PSPC before 1993, but it brightened substantially in 1993, with luminosities…

天体物理学 · 物理学 2009-11-07 Kajal Ghosh , Douglas Swartz , Allyn Tennant , Kinwah Wu

We observed the "micro-quasar" GRS 1758-258 four times with Chandra. Two HRC-I observations were made in 2000 September-October spanning an intermediate-to-hard spectral transition (identified with RXTE). Another HRC-I and an ACIS/HETGS…

天体物理学 · 物理学 2007-05-23 W. A. Heindl , D. M. Smith

This paper discusses the X-ray halo around the Swift gamma-ray burst GRB 050724 (z=0.258), detected by the Swift X-Ray Telescope. The halo, which forms a ring around the fading X-ray source, expands to a radius of 200" within 8 ks of the…

During a 50 ks monitoring observation of the Galactic bulge performed in September 1999 by the Wide Field Cameras on board the BeppoSAX satellite, an X-ray burst was detected from a sky position ~3 degrees off the Galactic centre. No…

天体物理学 · 物理学 2009-11-07 M. Cocchi , A. Bazzano , L. Natalucci , P. Ubertini , J. Heise , E. Kuulkers , R. Cornelisse , J. J. M. in 't Zand

Emission of two short hard X-ray bursts on 2009 June 5 disclosed the existence of a new soft gamma-ray repeater, now catalogued as SGR 0418+5729. After a few days, X-ray pulsations at a period of 9.1 s were discovered in its persistent…

We report the serendipitous discovery of a flare star observed with the ROSAT X-ray observatory. From optical spectra, which show strong and variable emission lines of the hydrogen Balmer series and neutral helium, we classify this object…

天体物理学 · 物理学 2015-06-24 J. D. Silverman , K. A. Eriksen , P. J. Green , S. H. Saar

We describe a series of observations of NGC 1313 using the ROSAT HRI with a combined exposure time of 183.5 ksec. The observations span an interval between 1992 and 1998; the purpose of observations since 1994 was to monitor the X-ray flux…

天体物理学 · 物理学 2009-10-31 Eric M. Schlegel , Robert Petre , E. J. M. Colbert , Scott Miller

SGR 1833-0832 was discovered on 2010 March 19 thanks to the Swift detection of a short hard X-ray burst and follow-up X-ray observations. Since then, it was repeatedly observed with Swift, Rossi X-ray Timing Explorer, and XMM-Newton. Using…

ROSAT HRI observations of 3C 273 reveal X-ray emission all along the optically visible jet with the peak of emission at the inner end. Whereas the X-ray emission from the innermost knot A is consistent with a continuation of the…

天体物理学 · 物理学 2007-05-23 Hermann-Josef Roeser , Klaus Meisenheimer , Martin Neumann , R. G. Conway , R. A. Perley

The results of GRANAT/SIGMA hard X-ray observations of GRS 1758-258 in 1990-1998 are presented. The source lies at ~5\arcdeg from the Galactic Center and was within the SIGMA field of view during the GRANAT surveys of this region. The total…

We report results from the analysis of XMM-Newton and INTEGRAL data of IGR J16479-4514. The unpublished XMM-Newton observation, performed in 2012, occurred during the source eclipse. No point-like X-ray emission was detected from the…

高能天体物理现象 · 物理学 2020-09-02 V. Sguera , A. Tiengo , L. Sidoli , A. J. Bird

We report on the X-ray spectral analysis and time evolution of GRS 1739$-$278 during its 2014 outburst based on MAXI/GSC and Swift/XRT observations. Over the course of the outburst, a transition from the low/hard state to the high/soft…

高能天体物理现象 · 物理学 2018-08-22 Sili Wang , Nobuyuki Kawai , Megumi Shidatsu , Yutaro Tachibana , Taketoshi Yoshii , Masayuki Sudo , Aya Kubota

We report results of a ROSAT High-Resolution Imager (HRI) observation of the X-ray error box given by the BeppoSAX Wide Field Camera for the gamma-ray burst that occurred on 1997 February 28. The observation started 10 days after the burst…

天体物理学 · 物理学 2007-05-23 F. Frontera , J. Greiner , L. A. Antonelli , E. Costa , F. Fiore , A. N. Parmar , L. Piro , T. Boller , W. Voges
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