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Related papers: The Black Hole Binary V4641 Sagitarii: Activity in…

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We present the spectral and timing evolution of the persistent black hole X-ray binary GRS 1758-258 based on almost 12 years of observations using the Rossi X-ray Timing Explorer Proportional Counter Array. While the source was…

The black hole candidate V4641 Sgr (= SAX J1819.3-2525) went through a brief outburst during 2003 Aug 01 to Aug 08. During the outburst, activity was noted in optical, radio as well as X-rays. Here we present results of Spectral and…

Astrophysics · Physics 2007-05-23 Dipankar Maitra , Charles D. Bailyn

We report results from a systematic study of X-ray emission from black hole transients in quiescence. In this state mass accretion is thought to follow the geometry of an outer optically thick, geometrically thin disc and an inner optically…

Astrophysics · Physics 2009-11-13 Gabor Pszota , Hui Zhang , Feng Yuan , Wei Cui

We study in detail the evolution of the 2015 outburst of GS 1354-64 (BW Cir) at optical, UV and X-ray wavelengths using Faulkes Telescope South/LCOGT, SMARTS and Swift. The outburst was found to stay in the hard X-ray state, albeit being…

High Energy Astrophysical Phenomena · Physics 2016-05-25 K. I. I. Koljonen , D. M. Russell , J. M. Corral-Santana , M. Armas Padilla , T. Muñoz-Darias , F. Lewis , M. Coriat , F. E. Bauer

We present a detailed study of optical data from the 2012 outburst of the candidate black hole X-ray binary Swift J1910.2-0546 using the Faulkes Telescope and Las Cumbres Observatory (LCO). We analyse the peculiar spectral state changes of…

High Energy Astrophysical Phenomena · Physics 2023-07-26 Payaswini Saikia , David M. Russell , Saarah F. Pirbhoy , M. C. Baglio , M. Bramich , Kevin Alabarta , Fraser Lewis , Phil Charles

In this paper we report on the optical and X-ray behaviour of the Be X-ray binary, SXP 91.1, during a recent type I outburst. We monitored the outburst using the Neil Gehrels Swift Observatory. These data were supported by optical data from…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Itumeleng Monageng , Malcolm Coe , Jamie Kennea , Lee Townsend , David Buckley , Vanessa McBride , Andrzej Udalski , Phil Evans , Paul Roche

Following the detection of a bright new X-ray source, MAXI J1659-152, a series of observations was triggered with almost all currently flying high-energy missions. We report here on XMM-Newton, INTEGRAL and RXTE observations during the…

We analyze a large set of new and archival photometric and spectroscopic observations of LMC X-3 to arrive at a self-consistent dynamical model for the system. Using echelle spectra obtained with the MIKE instrument on the 6.5m Magellan…

We present a detailed study of the long-timescale X-ray variability of the Narrow Line Seyfert 1 (NLS1) Galaxy MCG-6-30-15, based on 8 years of frequent observations with the Rossi X-ray Timing Explorer. Combined with short timescale…

Astrophysics · Physics 2009-11-10 I M McHardy , K F Gunn , P Uttley , M R Goad

IGR J17091-3624 is a distinctive black hole X-ray binary exhibiting exotic variability, including complex "heartbeat" oscillations in its X-ray light curves, similar to those observed in GRS 1915+105, a system renowned for its structured,…

GRS 1915$+$105 is a stellar-mass black hole that is well known for exhibiting at least 12 distinct classes of X-ray variability and correlated multi-wavelength behavior. Despite such extraordinary variability, GRS 1915$+$105 remained one of…

High Energy Astrophysical Phenomena · Physics 2021-03-10 Mayura Balakrishnan , J. M. Miller , M. T. Reynolds , E. Kammoun , A. Zoghbi , B. E. Tetarenko

We report on the results from Suzaku observations of the Galactic black hole X-ray binary H 1743-322 in the low/hard state during its outburst in 2012 October. We appropriately take into account the effects of dust-scattering to accurately…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Megumi Shidatsu , Yoshihiro Ueda , Shin'ya Yamada , Chris Done , Takafumi Hori , Kazutaka Yamaoka , Aya Kubota , Takahiro Nagayama , Yuki Moritani

The black hole candidate Swift J1753.5-0127 went into outburst in 2005 June. Rather than fade into quiescence as most black-hole-candidate transients do, it has remained in a low hard spectral state for most of the $\sim$ 9 years after…

High Energy Astrophysical Phenomena · Physics 2015-07-15 James Rodi , Elisabeth Jourdain , Jean-Pierre Roques

How black holes accrete surrounding matter is a fundamental, yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black holes via accretion disks, the state of which depends primarily on the…

The symbiotic X-ray binary 4U 1954+319 is a rare system hosting a peculiar neutron star (NS) and an M-type optical companion. Its ~5.4h NS spin period is the longest among all known accretion-powered pulsars and exhibited large (~7%)…

We describe the discovery of a solar neighborhood (d=468 pc) binary system with a main-sequence sunlike star and a massive non-interacting black hole candidate. The spectral energy distribution (SED) of the visible star is described by a…

We present the results of $WBVR$ observations of the low-mass X-ray binary V1341 $\textrm{Cyg} = \textrm{Cyg}$ X--2. Our observations include a total of 2375 individual measurements in four bands on 478 nights in 1986-1992. We tied the…

Solar and Stellar Astrophysics · Physics 2015-05-20 A. N. Sazonov

We have analyzed the X-ray spectra of the microquasar GRS 1915+105, as observed with the PCA on the Rossi XTE, during periods of stable weak emission, outbursts and rapid flaring. We find that the complicated X-ray intensity curve of this…

Astrophysics · Physics 2009-10-30 T. Belloni , M. Mendez , A. R. King , M. van der Klis , J. van Paradijs

We report the detection of the state transitions and hysteresis effect in the two mini-outbursts of the black hole (BH) transient GRS 1739$-$278 following its 2014 major outburst. The X-ray spectral evolutions in these two mini-outbursts…

High Energy Astrophysical Phenomena · Physics 2017-08-02 Zhen Yan , Wenfei Yu

We investigate the dependence of observational properties of black hole X-ray binaries on the inclination angle i of their orbits. We find the following: (1) Transient black hole binaries show no trend in their quiescent X-ray luminosities…

Astrophysics · Physics 2009-11-10 Ramesh Narayan , Jeffrey E. McClintock