In order to investigate the standard star solutions of the astrometric parameter determination in the FAST consortium, I developed an algorithm for the detection of astrometric binaries. The application of this algorithm was concentrated on those objects, where the Ø 2 -test of the astrometric parameter estimation using a single star model was not satisfactory. This method will be outlined in this paper. It is shown, that the accuracy of the Hipparcos observations allows the detection of brown dwarfs as a component of an astrometric binary. A systematic search of low mass companions among the M and K stars in the solar neighbourhood delivered six candidates possibly orbited by a brown dwarf, including Gliese 433. Key words: space astromet...
International audienceContext. The mass domain where massive extrasolar planets and brown dwarfs lie...
From radial velocity (RV) detections alone one does not get all orbital parameters needed to derive ...
The combination of Hipparcos astrometric data with the spectroscopic data of putative extrasolar pla...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
Context. The frequency of brown-dwarf companions in close orbit around Sun-like stars is l...
Context. The frequency of brown-dwarf companions in close orbit around Sun-like stars is low compare...
International audienceThe combination of Hipparcos astrometric data with the spectroscopic data of p...
International audienceThe combination of Hipparcos astrometric data with the spectroscopic data of p...
International audienceThe combination of Hipparcos astrometric data with the spectroscopic data of p...
The combination of Hipparcos astrometric data with the spectroscopic data of putative extrasolar pla...
The combination of Hipparcos astrometric data with the spectroscopic data of putative extrasolar pla...
International audienceContext. The mass domain where massive extrasolar planets and brown dwarfs lie...
International audienceContext. The mass domain where massive extrasolar planets and brown dwarfs lie...
From radial velocity (RV) detections alone one does not get all orbital parameters needed to derive ...
The combination of Hipparcos astrometric data with the spectroscopic data of putative extrasolar pla...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
International audienceThe orbital elements of 11 spectroscopic binaries with brown dwarf candidates ...
Context. The frequency of brown-dwarf companions in close orbit around Sun-like stars is l...
Context. The frequency of brown-dwarf companions in close orbit around Sun-like stars is low compare...
International audienceThe combination of Hipparcos astrometric data with the spectroscopic data of p...
International audienceThe combination of Hipparcos astrometric data with the spectroscopic data of p...
International audienceThe combination of Hipparcos astrometric data with the spectroscopic data of p...
The combination of Hipparcos astrometric data with the spectroscopic data of putative extrasolar pla...
The combination of Hipparcos astrometric data with the spectroscopic data of putative extrasolar pla...
International audienceContext. The mass domain where massive extrasolar planets and brown dwarfs lie...
International audienceContext. The mass domain where massive extrasolar planets and brown dwarfs lie...
From radial velocity (RV) detections alone one does not get all orbital parameters needed to derive ...
The combination of Hipparcos astrometric data with the spectroscopic data of putative extrasolar pla...