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相关论文: Transitions of black hole transients to the low/ha…

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We characterize the evolution of spectral and temporal properties of several Galactic black hole transients during outburst decay using the data from well sampled PCA/\rxte observations close to the transition to the low/hard state. We find…

天体物理学 · 物理学 2009-11-10 E. Kalemci , J. A. Tomsick , R. E. Rothschild , K. Pottschmidt , P. Kaaret

Multi-wavelength observations of Galactic black hole transients during outburst decay are instrumental for our understanding of the accretion geometry and the formation of outflows around black hole systems. H1743-322, a black hole…

天体物理学 · 物理学 2009-11-13 E. Kalemci , J. A. Tomsick , R. E. Rothschild , K. Pottschmidt , S. Corbel , P. Kaaret

A black hole spectrum is known to change from the hard state to the soft state when the energy spectral index $\alpha$ ($F_E \propto E^{-\alpha}$) in, say, 2-20 keV range changes from $\alpha \sim 0.5$ to $\sim 1.5$. However, this…

天体物理学 · 物理学 2007-05-23 Sandip K. Chakrabarti

Multiwavelength observations of Galactic black hole (GBH) transients during the state transitions and in the low/hard state may provide detailed information on the accretion structure of these systems. 4U1543-47 is a GBH transient that was…

We have analysed X-ray outbursts from several Galactic black hole (GBH) transients, as seen by the ASM on board RXTE. We have used the best estimates of distance and black hole mass to find their luminosity (scaled to the Eddington limit),…

天体物理学 · 物理学 2009-11-11 Marek Gierlinski , Jo Newton

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…

天体物理学 · 物理学 2009-11-07 E. Kalemci , J. A. Tomsick , R. E. Rothschild , K. Pottschmidt , S. Corbel , R. Wijnands , J. M. Miller , P. Kaaret

We present the results of the timing and color analysis of more than two hundred RXTE/PCA observations of the bright black-hole transient GX 339-4 obtained during its 2002/2003 outburst. The color-intensity evolution of the system, coupled…

天体物理学 · 物理学 2009-11-11 T. Belloni , J. Homan , P. Casella , M. van der Klis , E. Nespoli , W. H. G. Lewin , J. M. Miller , M. Mendez

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.…

天体物理学 · 物理学 2009-11-10 Sabrina Rossi , Jeroen Homan , Jon M. Miller , Tomaso Belloni

The results of X-ray observations of Galactic superluminal jet source GRS 1915+105 during its low luminosity state and state transitions in October, 1996 - April, 1997 with PCA and HEXTE instruments aboard Rossi X-ray Timing Explorer (RXTE)…

天体物理学 · 物理学 2007-05-23 S. Trudolyubov , E. Churazov , M. Gilfanov

In the study of black-hole transients, an important problem that still needs to be answered is how the high-energy part of the spectrum evolves from the low-hard to the high-soft state, given that they have very different properties. Recent…

高能天体物理现象 · 物理学 2015-05-14 Tomaso M. Belloni , Sara Motta

Here we report on Swift and Suzaku observations near the end of an outburst from the black hole transient 4U 1630-47 and Chandra observations when the source was in quiescence. 4U 1630-47 made a transition from a soft state to the hard…

高能天体物理现象 · 物理学 2015-06-22 John A. Tomsick , Kazutaka Yamaoka , Stephane Corbel , Emrah Kalemci , Simone Migliari , Philip Kaaret

We discuss the evolution of black hole transients on the basis of a few systems that were intensively observed with the Rossi X-ray Timing Explorer. We focus on the global evolution and the observed state transitions. Rather than giving a…

天体物理学 · 物理学 2011-09-29 Jeroen Homan , Tomaso Belloni

During the outbursts of black hole X-ray binaries (BHXRBs), their accretion flows transition through several states. The source luminosity rises in the hard state, dominated by non-thermal emission, before transitioning to the…

With the availability of the large database of black-hole transients from the Rossi X-Ray Timing Explorer, the observed phenomenology has become very complex. The original classification of the properties of these systems in a series of…

高能天体物理现象 · 物理学 2014-11-20 T. M. Belloni

We present the results of detailed analysis of X-ray data in 3-20 keV range from a ~70 day outburst of the neutron star transient Aquila X-1 during September-November 2000. Optical monitoring with the YALO 1m telescope was used to trigger…

天体物理学 · 物理学 2009-11-10 D. Maitra , C. D. Bailyn

We have used pointed RXTE data to examine the long-term X-ray light curves of six transient black hole X-ray binaries during their decay from outburst to quiescence. In most cases there is a period of exponential decay as the source…

高能天体物理现象 · 物理学 2015-05-27 Alexander Eckersall , Simon Vaughan , Graham Wynn

We examine the X-ray spectral and temporal behavior of the Galactic black hole candidate source GRS 1915+105 during its spectral state transition observed in 1997 March - August. The source was making a slow transition from a low-hard state…

天体物理学 · 物理学 2009-10-31 A. R. Rao , J. S. Yadav , B. Paul

We report on X-ray and soft gamma-ray observations of the black-hole candidate GX 339-4 during its 2007 outburst, performed with the RXTE and INTEGRAL satellites. The hardness-intensity diagram of all RXTE/PCA data combined shows a q-shaped…

Black hole transients are known to undergo spectral transitions that form q-shaped tracks on a hardness intensity diagram. In this work, we use archival RXTE data to extract a characteristic minimal timescale for the spectral states in GX…

高能天体物理现象 · 物理学 2020-09-30 E. Sonbas , K. Mohamed , K. S. Dhuga , A. Tuncer , E. Göğüş

We have discovered a spectral transition from the low/hard (LH) state to the high/soft (HS) state when Aquila X-1 was {\em declining} in observations made with the {\it Rossi X-Ray Timing Explorer (RXTE)}. The 2--200 keV energy flux…

天体物理学 · 物理学 2009-11-11 Wenfei Yu , Joshua Dolence
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