Open cluster kinematics with Gaia DR2 (Corrigendum)

@article{Soubiran2019OpenCK,
  title={Open cluster kinematics with Gaia DR2 (Corrigendum)},
  author={C. Soubiran and T. Cantat-Gaudin and Manuel Romero-G{\'o}mez and Laia Casamiquela and C. Jordi and Antonella Vallenari and T. Antoja and Lola Balaguer-N'unez and Diego Bossini and Angela Bragaglia and Ricardo Carrera and Alfred Castro-Ginard and Francesca Figueras and Ulrike Heiter and Daniel Martin Katz and Alberto Krone-Martins and J.-F. Le Campion and Andr{\'e} Moitinho and Rosanna Sordo},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
Context. Open clusters are very good tracers of the evolution of the Galactic disc. Thanks to Gaia, their kinematics can be investigated with an unprecedented precision and accuracy. Aims. The distribution of open clusters in the 6D phase space is revisited with Gaia DR2. Methods. The weighted mean radial velocity of open clusters was determined, using the most probable members available from a previous astrometric investigation that also provided mean parallaxes and proper motions. Those… Expand
Aggregates of clusters in the Gaia data
Context. The precision of the parallax measurements by Gaia is unprecedented. As of Gaia Data Release 2, the number of known nearby open clusters has increased. Some of the clusters appear to beExpand
The List of Possible Double and Multiple Open Clusters between Galactic Longitudes 240° and 270°
This work studies the candidate double and multiple open clusters (OCs) in the galactic sector from l = 240 o to l = 270 o , which contains the Vela-Puppis star formation region. To do that, we haveExpand

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