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相关论文: Infrared Jet of the Galactic Superluminal Source G…

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We observed the galactic microquasar GRS1915+105 in the K ($2.2 \mu$m) band on October 16 and 17, 1995 UTC using the COB infrared (IR) imager on the Kitt Peak National Observatory 2.1-m telescope with a 0.2-arcsec/pixel plate scale and…

天体物理学 · 物理学 2016-08-30 Stephen S. Eikenberry , Giovanni G. Fazio

Millimeter observations of the galactic source of relativistic ejections GRS 1915+105 (Mirabel & Rodriguez 1994) are consistent with this source being at a kinematic distance D = 12.5 +/- 1.5 kpc from the Sun, behind the core of a molecular…

天体物理学 · 物理学 2007-05-23 S. Chaty , I. F. Mirabel , P. -A. Duc , J. E. Wink , L. F. Rodríguez

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 report simultaneous observations in the X-ray, infrared, and radio wavelengths of the galactic superluminal source GRS 1915+105. During episodes of rapid disappearance and follow up replenishment of the inner accretion disk evidenced by…

天体物理学 · 物理学 2007-05-23 I. F. Mirabel , V. Dhawan , S. Chaty , L. F. Rodriguez , J. Marti , C. R. Robinson , J. Swank , T. Geballe

We present evidence that ~ 30 minute episodes of jet formation in the Galactic microquasar GRS 1915+105 may sometimes entirely be a superposition of smaller, faster phenomena. We base this conclusion on simultaneous X-ray and infrared…

天体物理学 · 物理学 2009-11-10 David M. Rothstein , Stephen S. Eikenberry , Keith Matthews

We present evidence that ~ 30 minute episodes of jet formation in GRS 1915+105 may sometimes be a superposition of smaller, faster phenomena. Based on observations in 2002 July using the Rossi X-ray Timing Explorer and the Palomar 5 meter…

天体物理学 · 物理学 2007-05-23 David M. Rothstein , Stephen S. Eikenberry , Keith Matthews

We report the discovery of fast (~ 100 sec) 2.2 micron flares from the microquasar GRS 1915+105, which are superimposed on longer (~ 30 min), brighter flares corresponding to episodes of jet formation. The number and strength of the…

天体物理学 · 物理学 2007-05-23 David M. Rothstein , Stephen S. Eikenberry

We have observed an extended region surrounding the first discovered galactic superluminal source GRS 1915+105, seeking evidence of interaction between the relativistic ejecta of that object and the interstellar medium. We find two radio…

天体物理学 · 物理学 2009-10-31 S. Chaty , L. F. Rodriguez , I. F. Mirabel , T. R. Geballe , Y. Fuchs , A. Claret , C. J. Cesarsky , D. Cesarsky

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 simultaneous X-ray and infrared (IR) observations of the Galactic microquasar GRS1915+105 using XTE and the Palomar 200-inch telescope on August 13-15, 1997 UTC. During the last two nights, the microquasar GRS 1915+105 exhibited…

天体物理学 · 物理学 2009-10-30 S. S. Eikenberry , K. Matthews , E. H. Morgan , R. A. Remillard , R. W. Nelson

We report simultaneous millimetre and infrared observations of a sequence of very large amplitude quasi-periodic oscillations from the black hole X-ray binary GRS 1915+105. These oscillations are near the end of a sequence of over 700…

天体物理学 · 物理学 2009-10-31 R. P. Fender , G. G. Pooley

The jets of GRS 1915+105 carry a considerable energy away from the central source into the ISM. The similarity of the jets of this source and jets in radio galaxies or radio-loud quasars suggests that we should detect large-scale,…

天体物理学 · 物理学 2009-11-10 Christian R. Kaiser , Katherine F. Gunn , Catherine Brocksopp , J. L. Sokoloski

We present GMRT observations of the Galactic microquasar GRS 1915+105 at 1.28 GHz for 8 days from 2001 June 18 to July 1. We have seen several isolated radio flares of varying magnitudes (20 - 50 mJy) and durations (6 - 35 min) and we model…

天体物理学 · 物理学 2009-11-07 C. H. Ishwara-Chandra , J. S. Yadav , A. Pramesh Rao

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 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 large mechanical luminosity of the jets of GRS 1915+105 should give rise to luminous emission regions, similar to those observed in radio galaxies, where the jets interact with the gas surrounding the source. However, no radio…

天体物理学 · 物理学 2009-11-10 Christian R. Kaiser , J. L. Sokoloski , Katherine F. Gunn , Catherine Brocksopp

We present the first detections of the black hole X-ray binary GRS 1915+105 at sub-millimetre wavelengths. We clearly detect the source at 350 GHz on two epochs, with significant variability over the 24 hr between epochs. Quasi-simultaneous…

天体物理学 · 物理学 2009-10-31 R. N. Ogley , S. J. Bell Burnell , R. P. Fender , G. G. Pooley , E. B. Waltman

We present multiwavelength observations of the superluminal jet source GRS 1915+105 in 1996 April-May, over which period a variety of phenomena, including radio QPO, strong infrared emission lines and rapid X-ray flickering and outbursts…

天体物理学 · 物理学 2007-05-23 R. P. Fender , G. G. Pooley , C. R. Robinson , B. A. Harmon , S. N. Zhang , C. Canosa

We present high resolution MERLIN radio images of multiple relativistic ejections from GRS 1915+105 in 1997 October / November. The observations were made at a time of complex radio behaviour, corresponding to multiple optically-thin…

We present 5-GHz MERLIN radio images of the microquasar GRS 1915+105 during two separate outbursts in 2001 March and 2001 July, following the evolution of the jet components as they move outwards from the core of the system. Proper motions…

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