Cl* NGC 104 LEE 8707 , the SIMBAD biblio

Cl* NGC 104 LEE 8707 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST06:45:30


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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.
2009A&A...505..117C viz 15       D               1 1554 734 Na-O anticorrelation and HB. VII. The chemical composition of first and second-generation stars in 15 globular clusters from GIRAFFE spectra. CARRETTA E., BRAGAGLIA A., GRATTON R.G., et al.
2009A&A...505..139C viz 16       D               1 225 517 Na-O anticorrelation and HB. VIII. Proton-capture elements and metallicities in 17 globular clusters from UVES spectra. CARRETTA E., BRAGAGLIA A., GRATTON R., et al.
2010ApJ...712L..21C viz 15       D               1 226 68 Calcium and light-elements abundance variations from high-resolution spectroscopy in globular clusters. CARRETTA E., BRAGAGLIA A., GRATTON R., et al.
2013A&A...550A..34C viz 15       D               1 261 36 An aluminium tool for multiple stellar generations in the globular clusters 47 Tucanae and M 4. CARRETTA E., GRATTON R.G., BRAGAGLIA A., et al.
2013ApJ...776...59D 15       D               1 30 14 Rubidium abundances in the globular clusters NGC 6752, NGC 1904, and NGC 104 (47 Tuc). D'ORAZI V., LUGARO M., CAMPBELL S.W., et al.
2013AJ....146..134K viz 15       D               1 419759 301 The radial velocity experiment (RAVE): fourth data release. KORDOPATIS G., GILMORE G., STEINMETZ M., et al.
2013A&A...558A..38M viz 15       D               1 57 31 FAMA: an automatic code for stellar parameter and abundance determination. MAGRINI L., RANDICH S., FRIEL E., et al.
2014ApJ...780...94C viz 15       D               1 184 88 Detailed abundances for a large sample of giant stars in the globular cluster 47 Tucanae (NGC 104). CORDERO M.J., PILACHOWSKI C.A., JOHNSON C.I., et al.
2017AJ....153...75K viz 16       D               1 451448 394 The Radial Velocity Experiment (RAVE): fifth data release. KUNDER A., KORDOPATIS G., STEINMETZ M., et al.
2017A&A...600A.104M viz 16       D               1 439 9 The potassium abundance in the globular clusters NGC 104, NGC 6752 and NGC 6809. MUCCIARELLI A., MERLE T. and BELLAZZINI M.
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.
2020Natur.583..768W viz 16       D               1 2060 39 The tidal remnant of an unusually metal-poor globular cluster. WAN Z., LEWIS G.F., LI T.S., et al.
2020AJ....160...83S viz 16       D               2 451375 83 The sixth Data Release of the Radial Velocity Experiment (RAVE). II. Stellar atmospheric parameters, chemical abundances, and distances. STEINMETZ M., GUIGLION G., McMILLAN P.J., 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...653A..13A viz 17       D               1 356 ~ Lithium in NGC 2243 and NGC 104. AOKI M., PRIMAS F., PASQUINI L., 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.
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...682A.126K 18       D               2 33 ~ Abundance of strontium in the Galactic globular cluster 47 Tuc. KOLOMIECAS E., KUCINSKAS A., KLEVAS J., et al.
2024A&A...685A..10S viz 18       D               1 234 ~ Heavy element abundances in galactic globular clusters. SCHIAPPACASSE-ULLOA J., LUCATELLO S., CESCUTTI G., et al.
2025A&A...699A..41S viz 19       D               1 255 ~ Neutron-capture element signatures in globular clusters Insights from the Gaia-ESO Survey. SCHIAPPACASSE-ULLOA J., MAGRINI L., LUCATELLO S., et al.

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