We report on the radio properties of jets of the following microquasars, as determined from daily multi-frequency monitoring observations with the RATAN-600 radio telescope during 2010–2017: V404 Cyg, SS433, Cyg X-1, GRS1915+105 and LSI+61 ∘ 303. We have detected many giant flares from SS433, a powerful flare from V404 Cyg in June 2015, an active state of Cyg X-1 in 2017 and fifty periodic flares from LSI+61 ∘ 303. We describe the properties of massive ejections based on multi-band (radio, X-ray and γ -ray) studies. The general properties of the light curves are closely connected with the processes of jet formation in microquasars
We discuss the results of the monitoring programs of the X-ray binaries with relativistic jets studi...
Super-massive black holes in active galaxies can accelerate particles to relativistic energies(1), p...
The microquasar V404 Cygni underwent a series of outbursts in 2015, June 15–31, during which its flu...
We report on the radio properties of jets of the following microquasars, as determined from daily mu...
© 2017 by the authors. We report on the radio properties of jets of the following microquasars, as d...
We present results of long-term daily monitoring of a sample of Galactic radio-emitting X-ray binari...
© 2017 by the authors. We report on two giant radio flares of the X-ray binary microquasar Cyg X-3, ...
We report on two giant radio flares of the X-ray binary microquasar Cyg X-3, consisting of a Wolf–Ra...
International audienceThe microquasar Cygnus X-3 underwent a giant radio flare in 2017 April, reachi...
The microquasar Cygnus X-3 underwent a giant radio flare in 2017 April, reaching a maximum flux of ∼...
Microquasars, X-ray binaries displaying relativistic jets driven by accretion onto a compact object,...
We report about the multi-frequency (1-30 GHz) daily monitoring of the radio flux variability of the...
Context. Microquasars are potential γ-ray emitters. Indications of transient episodes of γ-ray emiss...
Microquasars are potential γ-ray emitters. Indications of transient episodes of γ-ray emission were ...
We discuss the results of the monitoring programs of the X-ray binaries with relativistic jets studi...
Super-massive black holes in active galaxies can accelerate particles to relativistic energies(1), p...
The microquasar V404 Cygni underwent a series of outbursts in 2015, June 15–31, during which its flu...
We report on the radio properties of jets of the following microquasars, as determined from daily mu...
© 2017 by the authors. We report on the radio properties of jets of the following microquasars, as d...
We present results of long-term daily monitoring of a sample of Galactic radio-emitting X-ray binari...
© 2017 by the authors. We report on two giant radio flares of the X-ray binary microquasar Cyg X-3, ...
We report on two giant radio flares of the X-ray binary microquasar Cyg X-3, consisting of a Wolf–Ra...
International audienceThe microquasar Cygnus X-3 underwent a giant radio flare in 2017 April, reachi...
The microquasar Cygnus X-3 underwent a giant radio flare in 2017 April, reaching a maximum flux of ∼...
Microquasars, X-ray binaries displaying relativistic jets driven by accretion onto a compact object,...
We report about the multi-frequency (1-30 GHz) daily monitoring of the radio flux variability of the...
Context. Microquasars are potential γ-ray emitters. Indications of transient episodes of γ-ray emiss...
Microquasars are potential γ-ray emitters. Indications of transient episodes of γ-ray emission were ...
We discuss the results of the monitoring programs of the X-ray binaries with relativistic jets studi...
Super-massive black holes in active galaxies can accelerate particles to relativistic energies(1), p...
The microquasar V404 Cygni underwent a series of outbursts in 2015, June 15–31, during which its flu...