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The Gaia-ESO Survey : Membership probabilities for stars in 32 open clusters from 3D kinematics

Jackson, R. J. (author)
Keele University
Jeffries, R. D. (author)
Keele University
Wright, N. J. (author)
Keele University
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Randich, S. (author)
INAF - Osservatorio Astrofisico di Arcetri
Sacco, G. (author)
INAF - Osservatorio Astrofisico di Arcetri
Pancino, E. (author)
INAF - Osservatorio Astrofisico di Arcetri
Cantat-Gaudin, T. (author)
University of Barcelona
Gilmore, G. (author)
University of Cambridge
Vallenari, A. (author)
INAF - Osservatorio Astronomico di Padova
Bensby, T. (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Bayo, A. (author)
University of Valparaíso
Costado, M. T. (author)
University of Cádiz
Franciosini, E. (author)
INAF - Osservatorio Astrofisico di Arcetri
Gonneau, A. (author)
University of Cambridge
Hourihane, A. (author)
University of Cambridge
Lewis, J. (author)
University of Cambridge
Monaco, L. (author)
Andrés Bello National University
Morbidelli, L. (author)
INAF - Osservatorio Astrofisico di Arcetri
Worley, C. (author)
University of Cambridge
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 (creator_code:org_t)
2020-06-19
2020
English 16 s.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 496:4, s. 4701-4716
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • The Gaia-ESO Survey (GES) observed many open clusters as part of its programme to spectroscopically characterize the various Milky Way populations. GES spectroscopy and Gaia astrometry from its second data release are used here to assign membership probabilities to targets towards 32 open clusters with ages from 1 to 3800 Myr, based on maximum likelihood modelling of the 3D kinematics of the cluster and field populations. From a parent catalogue of 14 398 individual targets, 5032 stars with uniformly determined 3D velocities, Teff, log g, and chemistry are assigned cluster membership with probability >0.9, and with an average probability of 0.991. The robustness of the membership probabilities is demonstrated using independent membership criteria (lithium and parallax) in two of the youngest clusters. The addition of radial velocities improves membership discrimination over proper motion selection alone, especially in more distant clusters. The kinematically selected nature of the membership lists, independent of photometry and chemistry, makes the catalogue a valuable resource for testing stellar evolutionary models and investigating the time evolution of various parameters.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Open clusters and associations: general
Stars: evolution
Stars: pre-main-sequence

Publication and Content Type

art (subject category)
ref (subject category)

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