CCD Astrometry and Photometry of Visual Double Stars: Northern Hipparcos Wide Pairs Measured in the Years 2003-2005
DUCOURANT, C.
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Instituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] [IAG]
< Réduire
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Instituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] [IAG]
Langue
en
Communication dans un congrès
Ce document a été publié dans
Binary Stars as Critical Tools & Tests in Contemporary Astrophysics, Proceedings of IAU Symposium, Binary Stars as Critical Tools & Tests in Contemporary Astrophysics, Proceedings of IAU Symposium, Proceedings of IAU Symposium #240, held 22-25 August, 2006 in Prague, Czech Republic, 2006, Prague. 2006, vol. 240, p. 613-618
Edited by W.I. Hartkopf, E.F. Guinan and P. Harmanec. Cambridge: Cambridge University Press
Résumé en anglais
The relative positions of Hipparcos visual double star components are currently known with a precision around fifty mas. Modern CCD astrometric observations of these objects achieve an accuracy of their angular separation ...Lire la suite >
The relative positions of Hipparcos visual double star components are currently known with a precision around fifty mas. Modern CCD astrometric observations of these objects achieve an accuracy of their angular separation between ten and twenty mas per observation. New CCD measurements have been obtained at Kryonerion Observatory in the north hemisphere. They provide current relative positions of visual double stars which are at least twice as accurate as the ones provided by Hipparcos. The new measurements will permit us to extract the physical pairs from the sample, and the double stars, which have components of common origin. Final statistics of these systems will improve our understanding of stellar formation and evolution rates of wide binaries in the solar neighborhood.< Réduire
Mots clés en anglais
stars: wide double stars: Hipparcos
double stars
visual
astrometry
differential photometry
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