In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a long-term project focused on the search for new objects of this type. They performed a cross-identification between X-ray and radio catalogs under very restrictive selection criteria for sources with |b|<5 degrees, and obtained a sample of 13 radio-emitting X-ray sources. Follow-up observations of 6 of these sources with the VLA provided accurate coordinates, which were used to discover optical counterparts for all of them. We have observed these six sources with the EVN and MERLIN at 5 GHz. Five of the six objects have been detected and imaged, presenting different morphologies: one source has a two-sided jet, three sources have one-sided jet...
We present here new observations conducted with the EVN and MERLIN of the persistent microquasar LS ...
We present high angular resolution radio snap-shot observations of seven nearby low-luminosity activ...
Radio and X-ray observations have led to the presumption that some X-ray binaries (XRB) called micro...
In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a l...
In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a l...
In an attempt to increase the number of known microquasars, Paredes et al. ([CITE]) have presented a...
Recent studies of relativistic jet sources in the Galaxy, also known as microquasars, have been very...
Some microquasars are permanently bright radio sources while others are faint but produce powerful r...
We present here new observations conducted with the EVN and MERLIN of the persistent microquasar LS ...
Abstract Some microquasars are permanently bright radio sources while others are faint but produce p...
Aims.Microquasars are ideal natural laboratories for understanding accretion/ejection processes, st...
We present high-sensitivity 1.51 GHz e-MERLIN (e-Multi-Element Radio-Linked Interferometer Network) ...
Abstract. A series of observations of microquasar GRS1915+105 were made by the MERLIN telescope arra...
We present high-sensitivity 1.51 GHz e-MERLIN (e-Multi-Element Radio-Linked Interferometer Network) ...
We report optical spectroscopic observations of a sample of 6 low-galactic latitude microquasar cand...
We present here new observations conducted with the EVN and MERLIN of the persistent microquasar LS ...
We present high angular resolution radio snap-shot observations of seven nearby low-luminosity activ...
Radio and X-ray observations have led to the presumption that some X-ray binaries (XRB) called micro...
In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a l...
In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a l...
In an attempt to increase the number of known microquasars, Paredes et al. ([CITE]) have presented a...
Recent studies of relativistic jet sources in the Galaxy, also known as microquasars, have been very...
Some microquasars are permanently bright radio sources while others are faint but produce powerful r...
We present here new observations conducted with the EVN and MERLIN of the persistent microquasar LS ...
Abstract Some microquasars are permanently bright radio sources while others are faint but produce p...
Aims.Microquasars are ideal natural laboratories for understanding accretion/ejection processes, st...
We present high-sensitivity 1.51 GHz e-MERLIN (e-Multi-Element Radio-Linked Interferometer Network) ...
Abstract. A series of observations of microquasar GRS1915+105 were made by the MERLIN telescope arra...
We present high-sensitivity 1.51 GHz e-MERLIN (e-Multi-Element Radio-Linked Interferometer Network) ...
We report optical spectroscopic observations of a sample of 6 low-galactic latitude microquasar cand...
We present here new observations conducted with the EVN and MERLIN of the persistent microquasar LS ...
We present high angular resolution radio snap-shot observations of seven nearby low-luminosity activ...
Radio and X-ray observations have led to the presumption that some X-ray binaries (XRB) called micro...