Cl* NGC 6253 TAD 770 , the SIMBAD biblio

Cl* NGC 6253 TAD 770 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST11:50:06


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Title First 3 Authors
2003AJ....125.1383T viz 15       D               1 102 34 CCD uvbyCaHβ photometry of clusters. III. The most metal-rich open cluster, NGC 6253. TWAROG B.A., ANTHONY-TWAROG B.J. and DE LEE N.
2009A&A...505.1129M viz 15       D               1 3100 17 BVRIJHK photometry and proper motion analysis of NGC 6253 and the surrounding field. MONTALTO M., PIOTTO G., DESIDERA S., et al.
2010AJ....139.2034A viz 15       D               1 98 26 Wiyn open cluster study. XXXIX. Abundances in NGC 6253 from HYDRA spectroscopy of the Li 6708 Å region. ANTHONY-TWAROG B.J., DELIYANNIS C.P., TWAROG B.A., et al.
2012AJ....144..137C 15       D               1 58 20 Lithium abundances of the super-metal-rich open cluster NGC 6253. CUMMINGS J.D., DELIYANNIS C.P., ANTHONY-TWAROG B., et al.
2015AJ....149..141M 16       D               4 59 3 WIYN open cluster study. LXIII. Abundances in the super-metal-rich open cluster NGC 6253 from Hydra spectroscopy of the 7774 Å oxygen triplet region. MADERAK R.M., DELIYANNIS C.P., ANTHONY-TWAROG B.J., 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.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2021A&A...654A.137L viz 17       D               1 1739 4 The evolution of lithium in FGK dwarf stars. The lithium-rotation connection and the Li desert. LLORENTE DE ANDRES F., CHAVERO C., DE LA REZA R., et al.
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.
2024A&A...687A.124B viz 18       D               1 829 ~ The Gaia-ESO Survey: No sign of multiple stellar populations in open clusters from their sodium and oxygen abundances. BRAGAGLIA A., D'ORAZI V., MAGRINI L., et al.

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