Cl* NGC 104 LEE 1723 , the SIMBAD biblio

Cl* NGC 104 LEE 1723 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST01:43:37


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Title First 3 Authors
1992A&AS...93..293T viz 3072 38 Astrometry of globular clusters. I. Relative proper motions for stars in 47 Tuc. TUCHOLKE H.-J.
2001A&A...372...85R viz 227 29 Evolution of the dust mass loss with luminosity along the giant branch of the globular cluster 47 Tucanae. RAMDANI A. and JORISSEN A.
2017A&A...601A.112P viz 16       D               1 542 90 The Gaia-ESO Survey. Mg-Al anti-correlation in iDR4 globular clusters. PANCINO E., ROMANO D., TANG B., et al.
2018MNRAS.478.1520B viz 16       D               1 11619 300 A catalogue of masses, structural parameters, and velocity dispersion profiles of 112 Milky Way globular clusters. BAUMGARDT H. and HILKER M.
2020A&A...635A.155M viz 16       D               2 812 ~ The Gaia-ESO Survey: detection and characterisation of single-line spectroscopic binaries. MERLE T., VAN DER SWAELMEN M., VAN ECK S., et al.
2021A&A...656A..67D viz 17       D               1 263 ~ Abundance of barium in the atmospheres of red giants in the Galactic globular cluster NGC 104 (47 Tuc). DOBROVOLSKAS V., KOLOMIECAS E., KUCINSKAS A., et al.
2022MNRAS.509.1664J viz 17       D               1 14101 25 The Gaia-ESO Survey: Membership probabilities for stars in 63 open and 7 globular clusters from 3D kinematics. JACKSON R.J., JEFFRIES R.D., WRIGHT N.J., et al.
2022A&A...660A..46K viz 17       D               2 242 ~ Abundance of zirconium in the globular cluster 47 Tucanae: a possible Zr-Na correlation?*,**. KOLOMIECAS E., DOBROVOLSKAS V., KUCINSKAS A., 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...692A.228C viz 18       D               1 49864 ~ Inferring stellar parameters and their uncertainties from high-resolution spectroscopy using invertible neural networks. CANDEBAT N., SACCO G.G., MAGRINI L., et al.

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