2MASS J18545920-3028403 , the SIMBAD biblio

2MASS J18545920-3028403 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST23:02:44


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Title First 3 Authors
2010A&A...520A..95C viz 15       D               1 121 194 Detailed abundances of a large sample of giant stars in M 54 and in the Sagittarius nucleus. CARRETTA E., BRAGAGLIA A., GRATTON R.G., et al.
2017A&A...605A..46M viz 16       D               3 243 50 Chemical abundances in the nucleus of the Sagittarius dwarf spheroidal galaxy. MUCCIARELLI A., BELLAZZINI M., IBATA R., 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.
2020MNRAS.492.1641M viz 16       D               1 3434 81 Homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code - II. The Southern clusters and overview. MESZAROS S., MASSERON T., GARCIA-HERNANDEZ D.A., et al.
2020ApJ...889...63H viz 16       D               1 884 49 Metallicity and α-element abundance gradients along the Sagittarius stream as seen by APOGEE. HAYES C.R., MAJEWSKI S.R., HASSELQUIST S., et al.
2020AJ....160..120J viz 16       D               1 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021A&A...648A..70F 17       D               3 37 18 APOGEE spectroscopic evidence for chemical anomalies in dwarf galaxies: The case of M 54 and Sagittarius. FERNANDEZ-TRINCADO J.G., BEERS T.C., MINNITI D., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.

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