We briefly review the Galactic microquasar SS 433/W50 and present a new RXTE spectral and timing study. We show that the X-ray flux decreases during radio flares, a behavior seen in other microquasars. We also find short time-scale variability unveiling emission regions from within the binary system
In this paper we present our study of the gamma-ray emission from the microquasar SS433. Integrating...
We present Low-Frequency Array (LOFAR) high-band data over the frequency range 115-189 MHz for the X...
We report about the multi-frequency (1-30 GHz) daily monitoring of the radio flux variability of the...
We present X-ray images of all the available Chandra observations of the galactic jet source SS 433....
We present broad band power spectra of variations of SS433 in radio, optical and X-ray spectral band...
W50 remains the only supernova remnant (SNR) confirmed to harbor a microquasar: the powerful enigma...
© 2016, Pleiades Publishing, Inc.We study the X-ray variability of SS 433 based on data from the ASC...
We present an analysis of the X-ray data obtained in the period of flaring activity of SS 433 in Jul...
We present broad band power spectra of variations of SS433 in radio, optical and X-ray spectral band...
We present results of first simultaneous optical and X-ray observations of peculiar binary system SS...
Radio variability in some radio-quiet (RQ) active galactic nuclei suggests emission from regions clo...
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society....
The radio supernova remnant W50 hosts at its center the peculiar galactic X-ray binary SS 433. It sh...
We present results of long-term daily monitoring of a sample of Galactic radio-emitting X-ray binari...
We discuss the results of the monitoring programs of the X-ray binaries with relativistic jets studi...
In this paper we present our study of the gamma-ray emission from the microquasar SS433. Integrating...
We present Low-Frequency Array (LOFAR) high-band data over the frequency range 115-189 MHz for the X...
We report about the multi-frequency (1-30 GHz) daily monitoring of the radio flux variability of the...
We present X-ray images of all the available Chandra observations of the galactic jet source SS 433....
We present broad band power spectra of variations of SS433 in radio, optical and X-ray spectral band...
W50 remains the only supernova remnant (SNR) confirmed to harbor a microquasar: the powerful enigma...
© 2016, Pleiades Publishing, Inc.We study the X-ray variability of SS 433 based on data from the ASC...
We present an analysis of the X-ray data obtained in the period of flaring activity of SS 433 in Jul...
We present broad band power spectra of variations of SS433 in radio, optical and X-ray spectral band...
We present results of first simultaneous optical and X-ray observations of peculiar binary system SS...
Radio variability in some radio-quiet (RQ) active galactic nuclei suggests emission from regions clo...
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society....
The radio supernova remnant W50 hosts at its center the peculiar galactic X-ray binary SS 433. It sh...
We present results of long-term daily monitoring of a sample of Galactic radio-emitting X-ray binari...
We discuss the results of the monitoring programs of the X-ray binaries with relativistic jets studi...
In this paper we present our study of the gamma-ray emission from the microquasar SS433. Integrating...
We present Low-Frequency Array (LOFAR) high-band data over the frequency range 115-189 MHz for the X...
We report about the multi-frequency (1-30 GHz) daily monitoring of the radio flux variability of the...