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相关论文: ASCA and Ginga Observations of GX 1+4

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Centaurus X-3 is a persistent high-mass X-ray binary with the long-term light curve from the source exhibiting orbit-to-orbit intensity variations with no apparent superorbital periodicity. We used $\sim$13.5 years of MAXI/GSC data to study…

高能天体物理现象 · 物理学 2024-10-24 Ajith Balu , Kinjal Roy , Hemanth Manikantan , Abhisek Tamang , Biswajit Paul

We report on the March-April 1997 BeppoSAX observations of Aql X-1, the first to monitor the evolution of the spectral and time variability properties of a neutron star soft X-ray transient from the outburst decay to quiescence. We observed…

天体物理学 · 物理学 2009-10-30 S. Campana , L. Stella , S. Mereghetti , M. Colpi , M. Tavani , D. Ricci , D. Dal Fiume , T. Belloni

We detected an X-ray compact source inside the Cygnus Loop during the observation project of the whole Cygnus Loop with the ASCA GIS. The source intensity is 0.11 c s$^{-1}$ for GIS and 0.15 c s$^{-1}$ for SIS, which is the strongest in the…

天体物理学 · 物理学 2015-06-24 E. Miyata , H. Tsunemi , K. Torii , K. Hashimotodani , T. G. Tsuru , K. Koyama , K. Ayani , K. Ohta , M. Yoshida

We investigate the absorption and emission features in observations of GX 301-2 detected with Insight-HXMT/LE in 2017-2019. At different orbital phases, we found prominent Fe Kalpha, Kbeta and Ni Kalpha lines, as well as Compton shoulders…

We study gamma-ray observations of NGC 4151 by GRO/OSSE contemporaneous with X-ray observations by ROSAT and Ginga in 1991 June and with ASCA in 1993 May. The spectra are well modeled by thermal Comptonization and a dual neutral absorber.…

天体物理学 · 物理学 2015-06-24 A. A. Zdziarski , W. N. Johnson , P. Magdziarz

We report optical and IR observations of the ASCA X-ray pulsar system AX J0051-733. The relationship between the X-ray source and possible optical counterparts is discussed. Long term optical data from over 7 years are presented which…

天体物理学 · 物理学 2009-11-07 M. J. Coe , N. J. Haigh , S. G. T. Laycock , I. Negueruela , C. R. Kaiser

We present new X-ray spectral data for the Seyfert 1 nucleus in NGC 4151 observed with Chandra for 200 ks. A significant ACIS pileup is present, resulting in a non-linear count rate variation during the observation. With pileup corrected…

宇宙学与河外天体物理 · 物理学 2015-05-18 Junfeng Wang , G. Risaliti , G. Fabbiano , M. Elvis , A. Zezas , M. Karovska

We report on ASCA energy spectra of Cir X-1 taken near its zero phase on 1994 August 4-5. The ASCA SIS detectors allow a more detailed study of the iron K complex than has been possible before. We find that prior to a sudden upward flux…

天体物理学 · 物理学 2015-06-24 W. N. Brandt , A. C. Fabian , T. Dotani , F. Nagase , H. Inoue , T. Kotani , Y. Segawa

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…

PG1535+547 is a bright NLS1 galaxy, whose high energy emission shows strong variability in shape and flux. ROSAT data classified it as soft X-ray weak QSO (objects whose X-ray-to-optical flux ratio is smaller than in typical QSO): their…

天体物理学 · 物理学 2009-11-13 L. Ballo , M. Giustini , N. Schartel , M. Cappi , E. Jimenez-Bailon , E. Piconcelli , M. Santos-Lleo , C. Vignali

We report the transition to an active state of the nucleus in the Seyfert 1.9 galaxy NGC 2992, discovered by means of new hard X-ray data. While the 2-10 keV flux declined by a factor of ~ 20 from 1978 to 1994, two recent BeppoSAX…

天体物理学 · 物理学 2007-05-23 R. Gilli , R. Maiolino , A. Marconi , G. Risaliti , M. Dadina , K. A. Weaver , E. J. M. Colbert

We present a 2 - 10 keV ASCA observation of the field around the soft gamma repeater SGR1627-41. A quiescent X-ray source was detected in this observation whose position was consistent both with that of a recently discovered BeppoSAX X-ray…

The low energy (<10 keV) X-ray emission of the Soft Gamma-ray Repeater SGR1806-20 has been studied by means of four XMM-Newton observations carried out in the last two years, the latter performed in response to a strong sequence of hard…

天体物理学 · 物理学 2009-11-10 S. Mereghetti , A. Tiengo , P. Esposito , D. Gotz , L. Stella , G. L. Israel , N. Rea , M. Feroci , R. Turolla , S . Zane , -

The time-averaged 30 ks Chandra HETGS observation of the micro-quasar GRS 1915+105 in the low hard state reveals for the first time in this source neutral K absorption edges from Fe, Si, Mg, & S. Ionized resonance absorption from H-, and…

天体物理学 · 物理学 2009-11-07 J. C. Lee , C. S. Reynolds , N. S. Schulz , R. Remillard , E. G. Blackman , A. C. Fabian

The microquasar GX 339-4 was observed by Suzaku five times, spaced by a few days, during its transition back to the hard state at the end of its 2010-2011 outburst. The 2-10 keV source flux decreases by a factor ~10 between the beginning…

高能天体物理现象 · 物理学 2015-06-17 P. -O. Petrucci , C. Cabanac , S. Corbel , E. Koerding , R. Fender

AX J1749.1-2733 is an unclassified transient X-ray source discovered during surveys by ASCA in 1993-1999. A multi-wavelength study in NIR, optical, X-rays and hard X-rays is undertaken in order to determine its nature. AX J1749.1-2733 is a…

天体物理学 · 物理学 2008-09-08 J. A. Zurita Heras , S. Chaty

This paper presents a BeppoSAX observation of NGC 7582 made during 1998 November and an optical spectrum taken in 1998 October. The new X-ray data reveal a previously unknown hard X-ray component in NGC 7582, peaking close to 20 keV. Rapid…

天体物理学 · 物理学 2009-10-31 T. J. Turner , G. C. Perola , F. Fiore , G. Matt , I. M. George , L. Piro , L. Bassani

We present data from simultaneous Chandra, XMM-Newton and BeppoSAX observations of the Seyfert 1 galaxy NGC 3516, taken during 2001 April and Nov. We have investigated the nature of the very flat observed X-ray spectrum. Chandra grating…

天体物理学 · 物理学 2014-10-13 T. J. Turner , S. B. Kraemer , I. M. George , J. N. Reeves , M. C. Bottorff

Using data from the All Sky Monitor (ASM) on the Rossi X-ray Timing Explorer (RXTE) we have searched for long term periodicities in the X-ray flux of GX 1+4, Sco X-2 (GX 349+2), and GX 339-4. For GX 1+4 we also used data from BATSE and…

天体物理学 · 物理学 2010-03-26 Stefan Dieters , Paul O'Neill , Sean Farrell , Ravi Sood

We present a detailed re-analysis of the two {\it ASCA} Performance Verification observations of the nearby Seyfert 1 galaxy MCG-6-30-15. Confirming the results of Fabian et al. (1994), we find definite evidence for the {\sc O\,vii} and…

天体物理学 · 物理学 2015-06-24 C. S. Reynolds , A. C. Fabian , K. Nandra , H. Inoue , H. Kunieda , K. Iwasawa