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A RAVE investigation on Galactic open clusters I. Radial velocities and metallicities

Conrad, C; Scholz, R-D; Kharchenko, NV; Piskunov, AE; Schilbach, E; Roeser, S; Boeche, C; ... Siviero, A; + view all (2014) A RAVE investigation on Galactic open clusters I. Radial velocities and metallicities. Astronomy & Astrophysics , 562 , Article A54. 10.1051/0004-6361/201322070. Green open access

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Abstract

Context. Galactic open clusters (OCs) mainly belong to the young stellar population in the Milky Way disk, but are there groups and complexes of OCs that possibly define an additional level in hierarchical star formation? Current compilations are too incomplete to address this question, especially regarding radial velocities (RVs) and metallicities ([M/H]). Aims. Here we provide and discuss newly obtained RV and [M/H] data, which will enable us to reinvestigate potential groupings of open clusters and associations. Methods. We extracted additional RVs and [M/H] from the RAdial Velocity Experiment (RAVE) via a cross-match with the Catalogue of Stars in Open Cluster Areas (CSOCA). For the identified OCs in RAVE we derived and from a cleaned working sample and compared the results with previous findings. Results. Although our RAVE sample does not show the same accuracy as the entire survey, we were able to derive reliable for 110 Galactic open clusters. For 37 OCs we publish for the first time. Moreover, we determined for 81 open clusters, extending the number of OCs with by 69.

Type: Article
Title: A RAVE investigation on Galactic open clusters I. Radial velocities and metallicities
Open access status: An open access version is available from UCL Discovery
DOI: 10.1051/0004-6361/201322070
Publisher version: https://doi.org/10.1051/0004-6361/201322070
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: open clusters and associations: general / solar neighborhood / Galaxy: kinematics and dynamics / stars: kinematics and dynamics / stars: abundances
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10076784
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