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相关论文: The variable radio emission from GRS 1915+105

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Monitoring with the Ryle Telescope at 15 GHz of the Galactic X-ray transient source GRS 1915+105 has revealed a remarkable range of rapid and extended flares which appear to be related to the X-ray emission as recorded by the RXTE all-sky…

天体物理学 · 物理学 2007-05-23 G. G. Pooley , R. P. Fender

We report on extensive X-ray observations of the galactic superluminal motion source GRS 1915+105 with the RXTE satellite over the last year. More than 130 RXTE pointings have been performed. GRS 1915+105 displays drastic X-ray intensity…

天体物理学 · 物理学 2009-10-30 J. Greiner , E. Morgan , R. Remillard

We have compared simultaneous Ryle Telescope radio and Rossi X-Ray Timing Explorer X-ray observations of the galactic microquasar GRS 1915+105, using the classification of the X-ray behaviour in terms of three states as previously…

天体物理学 · 物理学 2009-11-07 M. Klein-Wolt , R. P. Fender , G. G. Pooley , T. Belloni , S. Migliari , E. H. Morgan , M. van der Klis

We combine a complete sample of 113 pointed observations taken with the Rossi X-ray Timing Explorer between 1996-1999, monitoring observations taken with the Ryle telescope and the Green Bank Interferometer, and selected observations with…

天体物理学 · 物理学 2009-11-06 M. P. Muno , R. A. Remillard , E. H. Morgan , E. B. Waltman , V. Dhawan , R. M. Hjellming , G. Pooley

The galactic superluminal motion source GRS 1915+105 was observed with RXTE at several occasions during its ongoing active state. The observed X-ray intensity changes drastically on a variety of time scales ranging from sub-seconds to days.…

天体物理学 · 物理学 2007-05-23 J. Greiner , E. H. Morgan , R. A. Remillard

Since the launch of INTEGRAL in late 2002 we have monitored the Galactic microquasar GRS 1915+105 with long exposures (~100 ks) pointings. All the observations have been conducted simultaneously with other instruments, in particular RXTE…

天体物理学 · 物理学 2007-05-23 J. Rodriguez , G. Pooley , D. C. Hannikainen , H. J. Lehto

The galactic superluminal motion source GRS 1915+105 has been extensively observed with the RXTE satellite over the last two years. More than 250 RXTE pointings have been performed until mid-May 1998 with more than 1.5 Msec exposure time on…

天体物理学 · 物理学 2009-10-30 J. Greiner , E. Morgan , R. Remillard

The galactic superluminal transient X-ray source GRS 1915+105 was observed with the pointed proportional counters (PPCs) onboard the Indian satellite IRS-P3 during 1996 July 23-27. We report here details of the behavior of this source…

天体物理学 · 物理学 2009-10-30 B. Paul , P. C. Agrawal , A. R. Rao

The radio emitting X-ray binary GRS 1915+105 shows a wide variety of X-ray and radio states. We present a decade of monitoring observations, with the RXTE-ASM and the Ryle Telescope, in conjunction with high-resolution radio observations…

星系天体物理 · 物理学 2015-05-14 A. Rushton , R. E. Spencer , G. Pooley , S. Trushkin

Since its discovery in 1992, the superluminal X-ray transient GRS 1915+105 has been extensively observed in an attempt to understand its behaviour. We present here first results from a multi-wavelength campaign undertaken from July to…

天体物理学 · 物理学 2009-10-30 R. Bandyopadhyay , P. Martini , E. Gerard , P. A. Charles , R. M. Wagner , C. Shrader , T. Shahbaz , I. F. Mirabel

(Abridged) We report the results of monitoring observations of the Galactic microquasar GRS 1915+105 performed simultaneously with INTEGRAL and RXTE Ryle . We present the results of the whole \integral campaign, report the sources that are…

We analyzed radio and X-ray observations of GRS 1915+105, between May 1995 and June 2006, focusing on the times characterized by radio flares and cycles of hard dips-soft spikes in the X-ray lightcurve. Assuming these flares to be discrete…

高能天体物理现象 · 物理学 2015-05-19 Lionel Prat , Jérôme Rodriguez , Guy Pooley

We have compared simultaneous Ryle Telescope (RT) radio and Rossi X-Ray Timing Explorer (RXTE) X-ray observations of the galactic microquasar GRS 1915+105. We find that radio emission, and therefore also the radio jet, requires the presence…

天体物理学 · 物理学 2007-05-23 M. Klein-Wolt , R. P. Fender , G. G. Pooley , T. Belloni , S. Migliari , E. H. Morgan , M. van der Klis

Powerful relativistic jets are one of the ubiquitous features of accreting black holes in all scales. GRS 1915+105 is a well-known fast-spinning black-hole X-ray binary with a relativistic jet, termed as a ``microquasar'', as indicated by…

GRS 1915+105 is a very well studied microquasar with a wide variety of temporal and spectral states. Multi-wavelength observations from radio to X-rays have uncovered clear relations between the variability in different bands. GRS 1915+105…

高能天体物理现象 · 物理学 2019-08-14 A. Szostek , G. Dubus , F. Brun , M. de Naurois

We report here the results of 2 observations performed simultaneously with INTEGRAL, RXTE, the Ryle and Nancay radio telescopes. These observations belong to the so-called $\nu$ and $\lambda$ classes of variability during which a high level…

天体物理学 · 物理学 2007-05-23 J. Rodriguez , G. Pooley , D. C. Hannikainen , H. J. Lehto

We report the X-ray observations of the Galactic X-ray transient source GRS 1915+105 with the PPCs of the Indian X-ray Astronomy Experiment(IXAE) onboard the Indian satellite IRS-P3 during 1997 June - August, which have revealed the…

天体物理学 · 物理学 2009-10-31 J. S. Yadav , A. R. Rao , P. C. Agrawal , B. Paul , S. Seetha , K. Kasturirangan

We report high sensitivity dual-frequency observations of radio oscillations from GRS 1915+105 following the decay of a major flare event in 2000 July. The oscillations are clearly observed at both frequencies, and the time-resolved…

天体物理学 · 物理学 2009-11-07 R. P. Fender , D. Rayner , S. A. Trushkin , K. O'Brien , R. J. Sault , G. G. Pooley , R. P. Norris

We have analyzed publicly available RXTE/PCAs archival data of GRS 1915+105 during its burst/flaring state. The burst cycle ranges from 30 to 1300 s. These bursts are different from the type I and type II classical bursts seen in Low Mass…

天体物理学 · 物理学 2009-11-06 J. S. Yadav , A. R. Rao

GRS 1915+105, one of the two known galactic microquasars, shows an extremely complex variability in the X-ray band, comparable to no other X-ray source in the sky. Making use of RXTE/PCA data, we have analyzed the X-ray spectral…

天体物理学 · 物理学 2015-06-24 T. Belloni , M. Mendez , A. R. King , M. van der Klis , J. van Paradijs
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