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Related papers: Multifrequency observations of XTE J0421+560/CI Ca…

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We present the results of the analysis of RXTE, BATSE and optical/infrared data of the 1998 outburst of the X-ray transient system XTE J0421+560 (CI Cam). The X-ray outburst shows a very fast decay (initial e-folding time ~0.5 days, slowing…

We report results of two BeppoSAX observations of the transient X-ray source XTE J0421+560 during the outburst that started in March 1998. The source exhibits radio jets and coincides with the binary system CI Cam. The 0.1--50 keV spectrum…

Astrophysics · Physics 2007-05-23 A. Orr , A. N. Parmar , M. Orlandini , F. Frontera , D. Dal Fiume , A. Segreto , A. Santangelo , M. Tavani

We report on a BeppoSAX observation of the transient X-ray source XTE J0421+560 during quiescence performed ~150 days after the 1998 April outburst. The source had an unabsorbed 0.5-10 keV flux of 6.7x10^{-12} erg/cm2/s and was still…

We present the results of observations of XTE J0421+560 X-ray transient with Rossi X-ray Timing Explorer in the beginning of April 1998. Lightcurve, obtained by ASM all-sky monitor, shows unusually fast decrease in the object's luminosity.…

Astrophysics · Physics 2007-05-23 M. Revnivtsev , A. Emelyanov , K. Borozdin

We report on BeppoSAX observations of the X-ray transient XTE J0421+560 in quiescence 156, 541, and ~690 days after the maximum of the 1998 April outburst. In the first observation the source was soft with a power-law photon index of 4.0…

Astrophysics · Physics 2007-05-23 A. N. Parmar , T. Belloni , M. Orlandini , D. Dal Fiume , A. Orr , N. Masetti

We report on timing and spectral observations of the microquasar XTE J1550-564 during its 2000 outburst made by the Rossi X-ray Timing Experiment (RXTE). We study the spectral properties of the source during both the rise to the outburst…

Astrophysics · Physics 2016-08-30 J. Rodriguez , S. Corbel , E. Kalemci , J. Tomsick

We present the results of the analysis of 11 RXTE/PCA observations of the January 2002 outburst of the black-hole transient XTE J1550-564. The outburst was rather short, with an e-folding time of ~11 days in the PCA band 3-25 keV. The…

Astrophysics · Physics 2009-11-07 T. Belloni , A. P. Colombo , J. Homan , S. Campana , M. van der Klis

We have investigated the Quasi Periodic Oscillation (QPO) properties of the transient accreting X-ray pulsar XTE J1858+034 during the second outburst of this source in April-May 2004. We have used observations made with the Proportional…

Astrophysics · Physics 2009-11-11 U. Mukherjee , S. Bapna , H. Raichur , B. Paul , S. N. A. Jaaffrey

We present optical and infrared monitoring of the 2005 outburst of the halo black hole X-ray transient XTE J1118+480. We measured a total outburst amplitude of ~5.7+-0.1 mag in the R band and ~5 mag in the infrared J, H and K_s bands. The…

We observed the newly discovered Galactic jet source XTE J0421+560 (= CI Cam) with ASCA from 1998 April 3.3 to April 4.1 (UT), three days after the beginning of the outburst. The X-ray intensity in the 1-10 keV band gradually decreased with…

Astrophysics · Physics 2009-10-31 Y. Ueda , M. Ishida , H. Inoue , T. Dotani , J. Greiner , W. H. G. Lewin

We present optical photometry and spectroscopy of the X-ray transient XTE J1859+226, obtained during outburst and its subsequent decay to quiescence. Both the X-ray and optical properties are very similar to those of well-studied black hole…

We present the long term X-ray light curves, detailed spectral and timing analyses of XTE J1908+094 using the Rossi X-ray Timing Explorer Proportional Counter Array observations covering two outbursts in 2002 and early 2003. At the onset of…

We report on the analysis of 8 years of MAssive Compact Halo Objects (MACHO) data for the source RX J0520.5-6932. A regular period of 24.4 days has been confirmed, however this is manifest almost entirely in the red part of the spectrum. A…

Astrophysics · Physics 2009-11-10 W. R. T. Edge , M. J. Coe , J. L. Galache , A. B. Hill

Galactic black hole transients show many interesting phenomena during outburst decays. We present simultaneous X-ray (RXTE, Swift, and INTEGRAL), and optical/near-infrared (O/NIR) observations (SMARTS) of the X-ray transient XTE J1752-223…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Y. Y. Chun , T. Dinçer , E. Kalemci , T. Güver , J. A. Tomsick , M. M. Buxton , C. Brocksopp , S. Corbel , A. Cabrera-Lavers

We investigate the timing behavior of XTE J1550-564 with the Rossi X-ray Timing Explorer (RXTE) as the source made a transition to the hard state during the decay of the 2000 outburst. We detect a high frequency QPO at 65 Hz in one…

We present multiwavelength observations of the newly discovered X-ray transient XTE J1118+480 obtained in the rising phase of the 2000 April outburst. This source is located at unusually high Galactic latitude and in a very low absorption…

Astrophysics · Physics 2009-10-31 R. I. Hynes , C. W. Mauche , C. A. Haswell , C. R. Shrader , W. Cui , S. Chaty

On 28 February 2007 a new outburst of the previously known transient source XTE J1856+053 was detected with RXTE/ASM. We present here the results of an XMM-Newton (0.5-10.0 keV) Target of Opportunity observation performed on 14 March 2007,…

Astrophysics · Physics 2011-08-31 G. Sala , J. Greiner , M. Ajello , N. Primak

X-ray irradiation in X-ray binaries is thought to control the behavior at the outer disc, which is observable mainly at optical wavelengths. It is generally parameterized phenomenologically, but it can also be predicted from theoretical…

High Energy Astrophysical Phenomena · Physics 2018-10-17 Mariko Kimura , Chris Done

We present spectroscopic observations of the X-ray transient XTE J1118+480 acquired during different epochs following the 2000 March outburst. We find that the emission line profiles show variations in their double-peak structure on time…

We present the results of the analysis of RXTE (Rossi X-ray Timing Explorer) observations of the new x-ray transient, SWIFT J1753.5-0127 during its outburst in July, 2005. The source was caught at the peak of the burst with a flux of…

Astrophysics · Physics 2008-11-26 M. C. Ramadevi , S. Seetha
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