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相关论文: Radio, Infrared and X-ray observations of GRS 1915…

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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

Multiple near-infrared wavelengths observations, carried out since 1993 on the galactic superluminal source of relativistic ejections GRS 1915+105, have yielded three important results. 1) The infrared counterpart of GRS 1915+105 exhibits…

天体物理学 · 物理学 2007-05-23 S. Chaty , I. F. Mirabel , L. F. Rodriguez , P. -A. Duc , M. Sauvage , A. J. Castro-Tirado , P. Callanan

We present the result of multi-wavelength observations of the microquasar GRS 1915+105 in a plateau state with a luminosity of ~7.5x10^{38) erg s-1 (~40% L_Edd), conducted simultaneously with the INTEGRAL and RXTE satellites, the ESO/NTT,…

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 present a progress report on MERLIN radio imaging of a radio outburst from GRS 1915+105. The major ejection occurred at the end of an approximately 20-day `plateau' state, characterised by low/hard X-ray fluxes and a relatively strong…

We present mid-infrared (4-18 micron) observations of the microquasar GRS 1915+105 obtained with ISOCAM, the camera on board the Infrared Space Observatory (ISO), in 1996 April and 1997 October. The first observation probably occurred…

天体物理学 · 物理学 2011-05-23 Yael Fuchs , I. Felix Mirabel , Arnaud Claret

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

A new class of X-ray sources was clearly established with the discovery of highly relativistic radio jets from the galactic sources GRS 1915+105 and GRO J1655-40. Both of these objects have given us a broader view of black holes and the…

天体物理学 · 物理学 2007-05-23 B. A. Harmon

The superluminal X-ray transient source GRS 1915+105 was observed during July 20-29, 1996 with the Indian X-ray Astronomy Experiment (IXAE) on the Indian satellite IRS-P3 launched on March 21, 1996 from Shriharikota Range in India. During…

天体物理学 · 物理学 2007-05-23 B. Paul , P. C. Agrawal , A. R. Rao

The two galactic `microquasars' with superluminal radio jets have been quite active during 1996, generatinga variety of studies involving both NASA and ground-based observatories. GRS~1915+105 has displayed dramatic accretion instability in…

We report imaging photometry of the radio-jet black hole candidate source GRS 1915+105 in the infrared K band. The observations reveal rapid infrared flare events on timescales of less than an hour. These events are strikingly similar to…

天体物理学 · 物理学 2016-01-13 R. P. Fender , G. G. Pooley , C. Brocksopp , S. J. Newell

We report infrared observations of the microquasar GRS 1915+105 using the NICMOS instrument of the Hubble Space Telescope during 9 visits in April-June 2003. During epochs of high X-ray/radio activity near the beginning and end of this…

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

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 investigate the association between the radio ``plateau'' states and the large superluminal flares in GRS 1915+105 and propose a qualitative scenario to explain this association. We identify several candidate superluminal flare events…

天体物理学 · 物理学 2009-11-10 S. V. Vadawale , A. R. Rao , S. Naik , J. S. Yadav , C. H. Ishwara-Chandra , A. Pramesh Rao , G. G. Pooley

GRS 1915+105 has exhibited at least three modes of long-wavelength (infrared to radio) flares. Class A flares are the bright ($\sim 1$ Jy) radio events whose apparent superluminal motion in many ways defines the microquasars. Class B flares…

天体物理学 · 物理学 2007-05-23 Stephen Eikenberry

We have carried out radio studies of the surroundings of the superluminal microquasar GRS~1915+105. Our main goal was to understand the possible relation of GRS~1915+105 with two infrared/radio sources that appear symmetrically located with…

天体物理学 · 物理学 2007-05-23 L. F. Rodriguez , I. Felix Mirabel

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

We present simultaneous infrared and X-ray observations of the Galactic microquasar GRS 1915+105 using the Palomar 5-m telescope and Rossi X-ray Timing Explorer on July 10, 1998 UT. Over the course of 5 hours, we observed 6 faint infrared…

天体物理学 · 物理学 2009-10-31 S. Eikenberry , K. Matthews , M. Muno , P. Blanco , E. Morgan , R. Remillard

We have observed microquasar GRS 1915+105 at 1.28 GHz for 8 days from June 18 to July 1, 2001 using Giant Metrewave Radio Telescope (GMRT). We have seen several isolated radio baby flares of varying intensity and duration. We have also…

天体物理学 · 物理学 2007-05-23 J. S. Yadav , C. H. Ishwara-Chandra , A. Pramesh Rao , G. G. Pooley
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