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相关论文: Class Transitions in Black Holes

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We characterized the evolution of spectral and temporal properties of several Galactic black hole transients observed between 1996-2001 using the data from well sampled PCA observations close to the transition to the low/hard state. We…

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

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

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

The Galactic microquasar GRS 1915+105 exhibits at least sixteen types of variability classes. Transitions from one class to another could take place in a matter of hours. In some of the classes, the spectral state transitions (burst-off to…

高能天体物理现象 · 物理学 2011-09-06 Partha Sarathi Pal , Sandip K. Chakrabarti , Anuj Nandi

The light curve of the galactic micro-quasar GRS 1915+105 changes in at least thirteen different ways which are called classes. We present examples of the transitions from one class to another as observed by the IXAE instrument aboard the…

天体物理学 · 物理学 2009-11-10 Sandip K. Chakrabarti , Anuj Nandi , A. K. Chatterjee , A. K. Choudhury , U. Chatterjee

A new accretion picture based on a small disk surrounding a black hole is developed for the wind-fed source Cyg X-1. The hard and soft spectral states of Cyg X-1 are interpreted in terms of co-spatial two component flows for the innermost…

高能天体物理现象 · 物理学 2018-07-11 Ronald E. Taam , Erlin Qiao , B. F. Liu , E. Meyer-Hofmeister

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 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

Accreting black holes radiate in one of several spectral states, switching from one to another for reasons that are as yet not understood. Using the best studied example, Cyg X-1, we identify the geometry and physical conditions…

天体物理学 · 物理学 2016-01-13 Juri Poutanen , Julian Krolik , Felix Ryde

Several galactic black holes show transitions between spectral states. In this paper we present a unifying radiation transfer model that can fit the spectral data in both states. We fit individual broad-band (from 1 keV up to 4 MeV)…

天体物理学 · 物理学 2007-05-23 Juri Poutanen , Paolo Coppi

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

We show that with the wind/jet activity, the spectral index of hard X-ray is changed in galactic microquasars. When mass loss takes place, the spectrum becomes softer and when mass gain takes place, the spectrum becomes harder. We present…

天体物理学 · 物理学 2016-11-09 Sandip K. Chakrabarti , A. Nandi , A. R. Rao

It has been a long-standing puzzle what triggers the spectral transition between the hard and soft states in Cyg X-1. Also, the origin of the frequently observed X-ray flares in the source still remains a mystery. In this paper, we will…

天体物理学 · 物理学 2007-05-23 Wei Cui , Wan Chen , S. N. Zhang

The well-known black hole X-ray binary GRS 1915+105 is a unique source in the sense that it cannot be classified within the standard picture of black hole binary states. In this work we study archival XMM-Newton observations taken between…

高能天体物理现象 · 物理学 2015-06-19 H. Stiele , W. Yu

We show that the model proposed by Esin, McClintock & Narayan (1997) for the low state, intermediate state and high state of the black hole soft X-ray transient, Nova Muscae 1991, is consistent with the spectral evolution of the black hole…

天体物理学 · 物理学 2009-10-30 Ann A. Esin , Ramesh Narayan , Wei Cui , J. Eric Grove , Shuang-Nan Zhang

To better constrain the emission mechanism underlying the hard state of galactic black hole candidates, we use high-time resolution RXTE lightcurves for Cyg X-1 and GX 399-4 to compute two higher order variability statistics for these…

天体物理学 · 物理学 2009-11-07 Thomas J. Maccarone , Paolo S. Coppi

In neutron star and black hole X-ray binaries the transitions between the two spectral states, hard and soft, signals the change between accretion via a hot advection-dominated flow(ADAF) and disk accretion. In a few cases the hard/soft…

天体物理学 · 物理学 2009-11-11 B. F. Liu , F. Meyer , E. Meyer-Hofmeister

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

GRS 1915+105 shows at least twelve distinct classes of light curves. By analysing the data obtained from Indian X-ray Astronomy Experiment (IXAE) instrument aboard IRS-P3 satellite, we show that in at least two days, transitions between one…

天体物理学 · 物理学 2009-11-10 Sandip K. Chakrabarti , A. Nandi , Asit Choudhury , Utpal Chatterjee

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…

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