SACCO, G. G.; SPINA, L.; RANDICH, S.; PALLA, F.; PARKER, R. J.; JEFFRIES, R. D.; JACKSON, R.; MEYER, M. R.; MAPELLI, M.; LANZAFAME, A. C.; BONITO, R.; DAMIANI, F.; FRANCIOSINI, E.; FRASCA, A.; KLUTSCH, A.; PRISINZANO, L.; TOGNELLI, E.; DEGL'INNOCENTI, S.; PRADA MORONI, P. G.; ALFARO, E. J.; MICELA, G.; PRUSTI, T.; BARRADO, D.; BIAZZO, K.; BOUY, H.; BRAVI, L.; LOPEZ-SANTIAGO, J.; WRIGHT, N. J.; BAYO, A.; GILMORE, G.; BRAGAGLIA, A.; FLACCOMIO, E.; KOPOSOV, S. E.; PANCINO, E.; CASEY, A. R.; COSTADO, M. T.; DONATI, P.; HOURIHANE, A.; JOFRE, P.; LARDO, C.; LEWIS, J.; MAGRINI, L.; MONACO, L.; MORBIDELLI, L.; SOUSA, S. G.; WORLEY, C. C.; ZAGGIA, S.

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SACCO, G. G.
Pôle Gérontologie

SPINA, L.

RANDICH, S.

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2017-01

Résumé en anglais

Table 1 lists the properties of the members of the young clusters Chamaeleon I observed by the Gaia-ESO Survey. The Table includes the common name to identify each star in the Gaia-ESO catalogue, the coordinates, the parameters used for the membership classification, the spectrograph (GIRAFFE or UVES) used in the observation, and if the star has been previously classified as member of this cluster. Table 2 lists the properties of the stars used for the structural analysis discussed in the paper. The Table includes the coordinates, the effective temperatures, the luminosities, if the parameters of the stars are retrieved from the literature or the Gaia-ESO catalogue and the masses. (2 data files).< Réduire

Mots clés en italien

Clusters: open

Radial velocities

Effective temperatures

Stars: masses

Origine

Importé de hal

Unités de recherche

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804