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相关论文: RXTE Observations of GRS 1915+105

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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 on long-term K band photometry of the galactic microquasar GRS 1915+105 since March 1999. We see variations of more than 1 mag, which are seemingly correlated with variations in X-ray intensity and spectral slope.

天体物理学 · 物理学 2007-05-23 J. Greiner , F. J. Vrba , A. A. Henden , H. H. Guetter , C. B. Luginbuhl

(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…

The Galactic black hole transient GRS1915+105 is famous for its markedly variable X-ray and radio behaviour, and for being the archetypal galactic source of relativistic jets. It entered an X-ray outburst in 1992 and has been active ever…

BeppoSAX observed GRS 1915+105 on October 2000 with a long pointing lasting about ten days. During this observation, the source was mainly in the rho class characterized by bursts with a recurrence time of between 40 and 100 s. We identify…

太阳与恒星天体物理 · 物理学 2015-05-30 T. Mineo , E. Massaro , A. D'Ai , F. Massa , M. Feroci , G. Ventura , P. Casella , C. Ferrigno , T. Belloni

We present data from the first of six monitoring Open Time observations of GRS 1915+105 undertaken with the orbiting INTEGRAL satellite. The source was clearly detected with all three X-ray and gamma-ray instruments on board. GRS 1915+105…

We report the discovery of two new types of variability in the neutron star low-mass X-ray binary MXB 1730-335 (the 'Rapid Burster'). In one observation in 1999, it exhibits a large-amplitude quasi-periodic oscillation with a period of…

高能天体物理现象 · 物理学 2015-06-24 T. Bagnoli , J. J. M. in 't Zand

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

Since its discovery in 1992, GRS 1915+105 has been among the brightest sources in the X-ray sky. However, in early 2018, it dimmed significantly and has stayed in this faint state ever since. We report on AstroSat and NuSTAR observation of…

高能天体物理现象 · 物理学 2024-02-12 Sajad Boked , Bari Maqbool , V. Jithesh , Ranjeev Misra , Naseer Iqbal , Yashpal Bhulla

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 here the first results of the spectral and timing analysis of our simultaneous INTEGRAL/RXTE observations of GRS 1915+105. The first observation ever performed with INTEGRAL revealed a new class of variability, where changes of…

天体物理学 · 物理学 2007-05-23 J. Rodriguez , D. C. Hannikainen , S. E. Shaw , C. Cabanac , Y. Fuchs

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

GRS 1915+105 is observed in an 'obscured' phase since May 2019, exhibiting steady and low X-ray luminosities, while being intervened by sporadic re-brightenings. In this work, we perform a comprehensive and wide-band analysis of the…

高能天体物理现象 · 物理学 2023-07-11 Athulya M. P. , Anuj Nandi

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

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…

高能天体物理现象 · 物理学 2021-03-10 Mayura Balakrishnan , J. M. Miller , M. T. Reynolds , E. Kammoun , A. Zoghbi , B. E. Tetarenko

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 present a temporal analysis of a BeppoSAX observation of GRS 1915+105 performed on April 13, 1999 when the source was in the rho class, which is characterised by quasi-regular bursting activity. The aim of the present work is to confirm…

高能天体物理现象 · 物理学 2016-01-27 T. Mineo , F. Massa , E. Massaro , A. D'Ai

We report a comprehensive study on spectral and timing properties of hard X-ray dips uniquely observed in some so-called variability classes of the micro-quasars GRS 1915+105 and IGR J17091-3624. These dips are characterized by a sudden…

高能天体物理现象 · 物理学 2015-06-17 Mayukh Pahari , J. S. Yadav , Jerome Rodriguez , Ranjeev Misra , Sudip Bhattacharyya , S. K. Pandey

The Galactic superluminal source GRS 1915+105 was found to experience a peculiar X-ray variability in a narrow count rate range of the PCA detector onboard RXTE. This can be seen as a ring-shaped pattern in the two-color diagram of count…

天体物理学 · 物理学 2009-10-30 Osmi Vilhu , Jukka Nevalainen

The extraordinarily long outburst of GRS 1915+105 makes it one of the most remarkable low-mass X-ray binaries (LMXBs). It has been in a state of constant outburst since its discovery in 1992, an eruption which has persisted ~100 times…

太阳与恒星天体物理 · 物理学 2010-06-25 P. Deegan , C. Combet , G. A. Wynn