Статья

Age determination for 269 <i>Gaia</i> DR2 open clusters

D. BossiniINAF–Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, 35122 Padova, ItalyA. VallenariINAF–Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, 35122 Padova, ItalyA. BragagliaINAF–Osservatorio di Astrofisica e Scienza dello Spazio, Via Gobetti 93/3, 40129 Bologna, ItalyT. Cantat-GaudinInstitut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí Franquès 1, 08028 Barcelona, SpainR. SordoINAF–Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, 35122 Padova, ItalyL. Balaguer-NúñezInstitut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí Franquès 1, 08028 Barcelona, SpainC. JordiInstitut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí Franquès 1, 08028 Barcelona, SpainA. MoitinhoSIM, Faculdade de Ciências, Universidade de Lisboa, Ed. C8, Campo Grande, 1749-016 Lisboa, PortugalC. SoubiranLaboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, Allée Geoffroy Saint-Hilaire, 33615 Pessac, FranceL. CasamiquelaLaboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, Allée Geoffroy Saint-Hilaire, 33615 Pessac, FranceR. CarreraINAF–Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, 35122 Padova, ItalyU. HeiterObservational Astrophysics, Department of Physics and Astronomy, Uppsala University, Box 516 75120 Uppsala, Sweden

2019en

ABI

Аннотация

Context . The Gaia Second Data Release provides precise astrometry and photometry for more than 1.3 billion sources. This catalog opens a new era concerning the characterization of open clusters and test stellar models, paving the way for better understanding of the disk properties. Aims . The aim of the paper is to improve the knowledge of cluster parameters, using only the unprecedented quality of the Gaia photometry and astrometry. Methods . We have made use of the membership determination based on the precise Gaia astrometry and photometry. We applied an automated Bayesian tool, BASE-9, to fit stellar isochrones on the observed G , G BP , G RP magnitudes of the high probability member stars. Results . We derive parameters such as age, distance modulus, and extinction for a sample of 269 open clusters, selecting only low reddening objects and discarding very young clusters, for which techniques other than isochrone-fitting are more suitable for estimating ages.

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Идентификаторы

DOI: 10.1051/0004-6361/201834693

Цитирования и источники

Цитирований: 2Использованных источников: 0

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