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Related papers: 'Spectro-temporal' variabilities and possible phys…

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We explored the `spectro - temporal' behaviour of outbursting Black Hole sources in X-rays, at the time of jet ejections which are observed as radio flares. The energy dependent evolution of the properties of all the sources studied, shows…

High Energy Astrophysical Phenomena · Physics 2013-12-13 D. Radhika , A. Nandi , S. Seetha

In this paper we study the relation of radio emission to X-ray spectral and variability properties for a large sample of black hole X-ray binary systems. This is done to test, refine and extend -- notably into the timing properties -- the…

High Energy Astrophysical Phenomena · Physics 2015-05-13 R. P. Fender , J. Homan , T. M. Belloni

We report on our attempt to understand the outbursting profile of Galactic Black Hole (GBH) sources, keeping in mind the evolution of temporal and spectral features during the outburst. We present results of evolution of Quasi-periodic…

High Energy Astrophysical Phenomena · Physics 2018-03-14 H. Sreehari , Anuj Nandi , D. Radhika , Nirmal Iyer , Samir Mandal

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

We study the spectral and temporal characteristics of the source GS 2023$+$338 (V404 Cyg) during the initial phase of its June 2015 outburst, over the energy range of 0.5 - 150 keV. This is the first detailed study of the characteristics of…

High Energy Astrophysical Phenomena · Physics 2016-08-31 Radhika D. , A. Nandi , V. K. Agrawal , S. Mandal

Due to the impressive amount of new data provided by the RXTE satellite in the past decade, our knowledge of the phenomenology of accretion onto black holes has increased considerably. In particular, it has been possible to schematize the…

Astrophysics · Physics 2009-11-11 Tomaso Belloni

Our knowledge of the phenomenology of accretion onto black holes has increased considerably thanks to ten years of observations with the RXTE satellite. However, only recently it has been possible to derive a scheme for the outburst…

Astrophysics · Physics 2008-11-26 Tomaso Belloni

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…

Astrophysics · Physics 2009-11-10 E. Kalemci , J. A. Tomsick , R. E. Rothschild , K. Pottschmidt , P. Kaaret

We study the effect of variable jet bulk Lorentz factors, i.e., either jet acceleration or deceleration, on partially synchrotron self-absorbed radio spectra from cores of radio-loud active galactic nuclei and black-hole binaries in the…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Andrzej A. Zdziarski

Episodic jets are usually observed in the intermediate state of black hole transients during their X-ray outbursts. Here we report the discovery of a strong positive correlation between the peak radio power of the episodic jet $P_{\rm jet}$…

High Energy Astrophysical Phenomena · Physics 2015-05-15 Hui Zhang , Wenfei Yu

We compiled the X-ray and soft gamma-ray observations of the Galactic black hole binary XTE J1859+226 in the 1999--2000 outburst from RXTE, ASCA, BeppoSAX and CGRO. Throughout systematic spectral analysis using a two-component model…

High Energy Astrophysical Phenomena · Physics 2024-12-05 Kazutaka Yamaoka , Toshihiro Kawaguchi , Michael L. McCollough , Ruben Farinelli , Sergei Trushkin

In the propagating oscillatory shock model, the oscillation of the post-shock region, i.e., the Compton cloud, causes the observed low-frequency quasi-periodic oscillations (QPOs). The evolution of QPO frequency is explained by the…

High Energy Astrophysical Phenomena · Physics 2016-09-27 Broja G. Dutta , Sandip K. Chakrabarti

We present a study of correlations between spectral and timing parameters for a sample of black hole X-ray binary candidates. Data are taken from GX 339-4, H 1743-322, and XTE J1650-500, as the Rossi X-ray Timing Explorer (RXTE) observed…

High Energy Astrophysical Phenomena · Physics 2015-06-12 H. Stiele , T. M. Belloni , E. Kalemci , S. Motta

we propose a jet model for the low/hard state of black-hole X-ray sources which explains a) the X-ray spectra, b) the timelag spectra, c) the increase in the amplitude (QPO and high frequency) with increasing photon energy, and d) the…

Astrophysics · Physics 2009-11-10 D. Giannios , N. D. Kylafis , D. Psaltis

We present results of recent observations and theoretical modeling of data from black holes accreting at very low luminosities (L/L_Edd ~ 10^{-8}). We discuss our newly developed time-dependent model for episodic ejection of relativistic…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Dipankar Maitra , Andrew Cantrell , Sera Markoff , Heino Falcke , Jon Miller , Charles Bailyn

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 investigated the relation between compact jet emission and X-ray variability properties of all black hole transients with multiwavelength coverage during their outburst decays. We studied the evolution of all power spectral components…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Tolga Dincer , Emrah Kalemci , John A. Tomsick , Michelle M. Buxton , Charles D. Bailyn

We study spectral and temporal properties of Galactic short orbital period transient black hole XTE J1118+480 during its 2005 outburst using archival data of RXTE PCA and HEXTE instruments in the combined energy range of $3-100$ keV.…

High Energy Astrophysical Phenomena · Physics 2020-12-02 Dipak Debnath , Debjit Chatterjee , Arghajit Jana , Sandip K. Chakrabarti , Kaushik Chatterjee

We show that outflow rates in jets directly depend on the spectral states of black holes. In particular, in soft states, when the Comptonized electrons are cold, outflow rate is close to zero. In hard states, outflow could be steady, but…

Astrophysics · Physics 2009-10-31 Sandip K. Chakrabarti

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
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