The variable radio emission from GRS 1915+105
arXiv:astro-ph/9708171 · doi:10.1093/mnras/292.4.925
Abstract
We present data on the monitoring of the Galactic X-ray transient GRS 1915+105 at 15 GHz with the Ryle Telescope. We have found quasi-periodic oscillations with periods in the range 20-40 min which are tentatively associated with the soft-X-ray variations on the same time-scale. The overall behaviour of the radio emission is shown to vary in a strong association with the X-ray emission as recorded by the RXTE all-sky monitor.
Seven pages, five figures. Accepted for publication in MNRAS
Cited by in corpus (116)
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- The radio/X-ray correlation in Cyg X-3 and the nature of its hard spectral state
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- Evidence for deceleration in the radio jets of GRS1915+105?
- Long-term multi-wavelength studies of GRS 1915+105 I. A high-energy and mid-infrared focus with RXTE, INTEGRAL, and Spitzer
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- Disk-Jet Connection in the Microquasar GRS 1915+105 and IR and Radio Emission
- Opacity effects and shock-in-jet modelling of low-level activity in Cygnus X-3
- Evidence for local mass accretion rate variations in the disc of GRS 1915+105
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- Is the plateau state in GRS 1915+105 equivalent to canonical hard states?
- Stochastic variability in X-ray emission from the black hole binary GRS 1915+105
- Mid-Infrared observations of GRS 1915+105 during plateau and flaring states
- RXTE Spectroscopy of GRS 1915+105
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- The evolution of the high-frequency variability in the black hole candidate GRS 1915+105 as seen by RXTE
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- Circularly polarised radio emission from GRS 1915+105 and other X-ray binaries
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