Cl* Collinder 110 DI 1122 , the SIMBAD biblio

Cl* Collinder 110 DI 1122 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST08:50:36


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Title First 3 Authors
1998AJ....115.1076D viz 537 7 Collinder 110: an old open cluster in Monoceros. DAWSON D.W. and IANNA P.A.
2014AJ....147..138C viz 15       D               1 450 12 Rotational and radial velocities of 1.3-2.2 M☉ red giants in open clusters. CARLBERG J.K.
2015MNRAS.446.3651M 54 49 New insights on Ba overabundance in open clusters. Evidence for the intermediate neutron-capture process at play? MISHENINA T., PIGNATARI M., CARRARO G., et al.
2018A&A...618A..93C viz 16       D               1 87620 517 A Gaia DR2 view of the open cluster population in the Milky Way. CANTAT-GAUDIN T., JORDI C., VALLENARI A., et al.
2020A&A...633A..99C viz 16       D               1 257585 169 Clusters and mirages: cataloguing stellar aggregates in the Milky Way. CANTAT-GAUDIN T. and ANDERS F.
2020A&A...640A...1C viz 16       D               1 235399 241 Painting a portrait of the Galactic disc with its stellar clusters. CANTAT-GAUDIN T., ANDERS F., CASTRO-GINARD A., et al.
2021A&A...647A..19T viz 17       D               1 24814 55 3D kinematics and age distribution of the open cluster population. TARRICQ Y., SOUBIRAN C., CASAMIQUELA L., et al.
2021A&A...651A..84M viz 17       D               1 11678 30 The Gaia-ESO survey: Mixing processes in low-mass stars traced by lithium abundance in cluster and field stars. MAGRINI L., LAGARDE N., CHARBONNEL C., et al.
2021A&A...655A..23M viz 17       D               1 311 15 Gaia-ESO survey: Lithium abundances in open cluster Red Clump stars. MAGRINI L., SMILJANIC R., FRANCIOSINI E., et al.
2022ApJ...929...29G viz 17       D               1 8982 ~ Detection of Gravitational Redshift in Open Cluster Nondegenerate Stars. GUTIERREZ C.M. and RAMOS-CHERNENKO N.
2023A&A...676A.129H viz 17       D               1 114943 ~ The Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances. HOURIHANE A., FRANCOIS P., WORLEY C.C., et al.

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