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- Title
Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution.
- Authors
Cantat-Gaudin, T.; Vallenari, A.; Sordo, R.; Pensabene, F.; Krone-Martins, A.; Moitinho, A.; Jordi, C.; Casamiquela, L.; Balaguer-Núnez, L.; Soubiran, C.; Brouillet, N.
- Abstract
Context. The Tycho-Gaia Astrometric Solution (TGAS) subset of the first Gaia catalogue contains an unprecedented sample of proper motions and parallaxes for two million stars brighter than G ~ 12 mag. Aims. We take advantage of the full astrometric solution available for those stars to identify the members of known open clusters and compute mean cluster parameters using either TGAS or the fourth U.S. Naval Observatory CCD Astrograph Catalog (UCAC4) proper motions, and TGAS parallaxes. Methods. We apply an unsupervised membership assignment procedure to select high probability cluster members, we use a Bayesian/Markov Chain Monte Carlo technique to fit stellar isochrones to the observed 2MASS JHKS magnitudes of the member stars and derive cluster parameters (age, metallicity, extinction, distance modulus), and we combine TGAS data with spectroscopic radial velocities to compute full Galactic orbits. Results. We obtain mean astrometric parameters (proper motions and parallaxes) for 128 clusters closer than about 2 kpc, and cluster parameters from isochrone fitting for 26 of them located within a distance of 1 kpc from the Sun. We show the orbital parameters obtained from integrating 36 orbits in a Galactic potential.
- Subjects
OPEN clusters of stars; MARKOV chain Monte Carlo; RADIAL velocity of stars; PROPER motion of stars; STELLAR orbits
- Publication
Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, Vol 615, p1
- ISSN
0004-6361
- Publication type
Article
- DOI
10.1051/0004-6361/201731251