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We report on the evolution of the X-ray energy spectrum for the black hole candidate (BHC) X-ray transient XTE J1550-564 during the decay of the 2000 outburst. The Rossi X-ray Timing Explorer (RXTE) and Chandra observations span nearly five…

Astrophysics · Physics 2009-11-06 John A. Tomsick , Stephane Corbel , Philip Kaaret

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 report on timing and spectral observations of the 2000 outburst of XTE J1550-564 made by the Unconventional Stellar Aspect (USA) Experiment on board the Advanced Research and Global Observation Satellite (ARGOS). We observe a…

We re-investigated the `spectro-temporal' behaviour of the source XTE J1859+226 in X-rays during its outburst phase in 1999, by analysing the RXTE PCA/HEXTE data in 2 - 150 keV spectral band. Detailed analysis shows that although the…

High Energy Astrophysical Phenomena · Physics 2015-06-16 D. Radhika , A Nandi

On two occasions, we obtained nearly simultaneous ~ 4 kilosecond snapshot observations of the Galactic black hole and microquasar XTE J1550-564 with Chandra and RXTE near the peak of its May, 2000 outburst. The low-energy sensitivity of…

We follow the evolution of a low frequency QPO during the 2000 outburst of the microquasar XTE J1550-564, which was found to be present in the PCA energy range (2-65 keV) in 19 of 43 observations. The frequency of the QPO varies from 0.1 Hz…

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

Excellent coverage of the entire 16-month 1996-97 outburst cycle of GRO J1655-40 was provided by RXTE. We present a full spectral analysis of these data, which includes 52 PCA spectra from 2.5-20 keV and HEXTE spectra above 20 keV. We also…

We present results of spectral and timing analysis based on 11 RXTE PCA/HEXTE observations of the microquasar XTE J1550-564 during its last outburst in January 2002. The observed behaviour is comparable to most Black-Hole Candidates in the…

Astrophysics · Physics 2007-05-23 A. P. Colombo , T. Belloni , J. Homan , S. Campana , M. van der Klis

We present an analysis of the RXTE observations of the recently discovered Galactic microquasar XTE J1748--288 during its 1998 outburst. The spectral evolution of the source during the outburst can be considered a sequence of qualitatively…

Astrophysics · Physics 2009-10-31 M. G. Revnivtsev , S. P. Trudolyubov , K. N. Borozdin

We study the time variability and spectral evolution of the Black Hole Candidate source XTE J1650-500 using the BeppoSax wide energy range (0.12-200 keV) observations performed during the 2001 X-ray outburst. The source evolves from a…

Astrophysics · Physics 2011-02-11 Enrico Montanari , Lev Titarchuk , Filippo Frontera

The onset of most microquasar outbursts is characterized by a state transition between a Low/Hard State (LHS) and a High/Soft State (HSS). Besides drastic spectral and timing changes, this transition often shows a discrete ejection event…

High Energy Astrophysical Phenomena · Physics 2009-06-25 Lionel Prat , Jerome Rodriguez

We study the evolution of some microquasars during their outbursts as observed with the X-ray telescopes RXTE and INTEGRAL. We focus on the interplay between the accretion disc, and the medium responsible for the production of the hard…

Astrophysics · Physics 2010-04-30 Jerome Rodriguez , Lionel Prat

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 a study of the X-ray transient and black hole candidate XTE J1650-500 during its 2001/2002 outburst. The source made two state transitions between the hard and soft states, at luminosity levels that differed by a factor of ~5-10.…

Astrophysics · Physics 2009-11-10 Sabrina Rossi , Jeroen Homan , Jon M. Miller , Tomaso Belloni

Using the Chandra X-ray Observatory and the Rossi X-ray Timing Explorer, we have studied the black hole candidate (BHC) X-ray transient XTE J1650-500 near the end of its 2001-2002 outburst after its transition to the low-hard state at X-ray…

Astrophysics · Physics 2009-11-10 John A. Tomsick , Emrah Kalemci , Philip Kaaret

We report on RXTE observations of the microquasar XTE J1550 during a ~70 day outburst in April-June 2000. We focus here on the temporal properties of the source and study the behavior of low frequency (0.1-10 Hz) quasi periodic oscillations…

Astrophysics · Physics 2009-11-10 J. Rodriguez , S. Corbel , E. Kalemci , J. A. Tomsick , M. Tagger

Evolution of variability properties of Galactic transient sources is a diagnostic tool to understand various regimes of the accretion flow and its dynamics close to the central black hole. In this paper, we concentrate on the variability…

High Energy Astrophysical Phenomena · Physics 2020-08-11 Arka Chatterjee , Broja G. Dutta , Prantik Nandi , Sandip K. Chakrabarti

We investigated the temporal behavior of the new black hole transient XTE J1650-500 with the Rossi X-ray Timing Explorer (RXTE) as the source made a transition to the low/hard state during the decay of the 2001 outburst. We find QPOs in the…

We study the spectral properties of the first 14 observations of the rise to outburst phase of the X-ray transient J1550-564. Using the PCA and HEXTE instruments, we find that the 3-200 keV spectra smoothly pass from a standard low/hard…

Astrophysics · Physics 2009-11-06 Colin D. Wilson , Chris Done
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