We report Hipparcos observations of a number of binary systems, symbiotic stars and bright long period binaries, which are known also for being radio sources. In these systems the matter ejected from the component(s) is generally made visible in the radio by the ionizing radiation of the hot component of the system. Shocks from wind collision may also play a role, especially in those objects which are known for being X--ray sources. Hipparcos has shown that in most cases the astrometric position is very close to the core of the radio source. In particular, in the case of multiple radio sources, the Hipparcos position is close to the central source of CH Cyg, to the brightest source of AG Dra, and to the SiO maser emission of R Aqr. Key word...
Optical positions relative to the Hipparcos Catalogue (ESA 1997) have been obtained for the optical...
International audienceThe Hipparcos Catalogue contains astrometric results for 117 955 catalogue ent...
Artículo de publicación ISIWe present multifrequency, matching-beam, VLA radio continuum observation...
We report the 6-cm radio-continuum detection of a previously unknown radio star, HIP 68718, identifi...
Subarcsecond ( ~0\u27:3 x ~0\u27:1) observations of the RX Puppis symbiotic system with the Very Lar...
Radio emission has been detected from all the stages of stellar evolution across the HR diagram. Its...
Using the absolute astrometric positions and proper motions for common stars in the Hipparcos and Ga...
peer reviewedThe multiplicity of massive stars is known to be significantly high. Even though the ma...
Multi-frequency observations using a wide variety of telescopes and instrumentation have been used t...
We report evidence for ~1 extended structure in 6 cm continuum emission emanating from the symbioti...
[eng] High-mass binary systems involve extreme environments that produce non-thermal emission from r...
In order to contribute to the alignment of the radio and optical reference frames, 50 stars with con...
Context. Radio observations are an effective tool for discovering particle acceleration regions in c...
A survey for radio emission at 6 GHz and 9 GHz toward three regions of massive star formation in the...
From speckle observations made with the PISCO speckle camera at the Pic du Midi Observatory, we pre...
Optical positions relative to the Hipparcos Catalogue (ESA 1997) have been obtained for the optical...
International audienceThe Hipparcos Catalogue contains astrometric results for 117 955 catalogue ent...
Artículo de publicación ISIWe present multifrequency, matching-beam, VLA radio continuum observation...
We report the 6-cm radio-continuum detection of a previously unknown radio star, HIP 68718, identifi...
Subarcsecond ( ~0\u27:3 x ~0\u27:1) observations of the RX Puppis symbiotic system with the Very Lar...
Radio emission has been detected from all the stages of stellar evolution across the HR diagram. Its...
Using the absolute astrometric positions and proper motions for common stars in the Hipparcos and Ga...
peer reviewedThe multiplicity of massive stars is known to be significantly high. Even though the ma...
Multi-frequency observations using a wide variety of telescopes and instrumentation have been used t...
We report evidence for ~1 extended structure in 6 cm continuum emission emanating from the symbioti...
[eng] High-mass binary systems involve extreme environments that produce non-thermal emission from r...
In order to contribute to the alignment of the radio and optical reference frames, 50 stars with con...
Context. Radio observations are an effective tool for discovering particle acceleration regions in c...
A survey for radio emission at 6 GHz and 9 GHz toward three regions of massive star formation in the...
From speckle observations made with the PISCO speckle camera at the Pic du Midi Observatory, we pre...
Optical positions relative to the Hipparcos Catalogue (ESA 1997) have been obtained for the optical...
International audienceThe Hipparcos Catalogue contains astrometric results for 117 955 catalogue ent...
Artículo de publicación ISIWe present multifrequency, matching-beam, VLA radio continuum observation...