BPS CS 29518-0020 , the SIMBAD biblio

BPS CS 29518-0020 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST05:58:17

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2004A&A...422..527S viz 500 36 uvby-β photometry of high-velocity and metal-poor stars. X. Stars of very low metal abundance: Observations, reddenings, metallicities, classifications, distances, and relative ages. SCHUSTER W.J., BEERS T.C., MICHEL R., et al.
2007ApJS..168..128B viz 15       D               1852 38 Broadband UBVRCIC photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I. BEERS T.C., FLYNN C., ROSSI S., et al.
2007A&A...462..851B 3         O           35 213 First stars. VII - Lithium in extremely metal poor dwarfs. BONIFACIO P., MOLARO P., SIVARANI T., et al.
2007A&A...464.1081A 55 100 NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars. ANDRIEVSKY S.M., SPITE M., KOROTIN S.A., et al.
2008A&A...481..481A 16       D               1 52 114 NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars. ANDRIEVSKY S.M., SPITE M., KOROTIN S.A., et al.
2009ApJ...698.1803A 17       D               2 31 144 Lithium abundances of extremely metal-poor turnoff stars. AOKI W., BARKLEM P.S., BEERS T.C., et al.
2009A&A...501..519B viz 16       D               4 58 187 First stars. XII. Abundances in extremely metal-poor turnoff stars, and comparison with the giants. BONIFACIO P., SPITE M., CAYREL R., et al.
2010A&A...509A..88A 15       D               1 54 90 Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Milky way. ANDRIEVSKY S.M., SPITE M., KOROTIN S.A., et al.
2010A&A...512A..54C viz 15       D               1 465 610 An absolutely calibrated Teff scale from the infrared flux method. Dwarfs and subgiants. CASAGRANDE L., RAMIREZ I., MELENDEZ J., et al.
2010A&A...515L...3M 53       D     X         2 90 139 Observational evidence for a broken Li spite plateau and mass-dependent Li depletion. MELENDEZ J., CASAGRANDE L., RAMIREZ I., et al.
2010A&A...515A.111S viz 15       D               2 17230 227 The PASTEL catalogue of stellar parameters. SOUBIRAN C., LE CAMPION J.-F., CAYREL DE STROBEL G., et al.
2010A&A...522A..26S viz 20       D   O           4 36 369 The metal-poor end of the Spite plateau. I. Stellar parameters, metallicities, and lithium abundances. SBORDONE L., BONIFACIO P., CAFFAU E., et al.
2012A&A...541A.143S viz 15       D               1 55 38 NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars. SPITE M., ANDRIEVSKY S.M., SPITE F., et al.
2013ApJ...762...26Y viz 16       D               1 198 263 The most metal-poor stars. II. Chemical abundances of 190 metal-poor stars including 10 new stars with [Fe/H] ≤ -3.5. YONG D., NORRIS J.E., BESSELL M.S., et al.
2013A&A...551A..57H 16       D   O           1 73 63 LTE or non-LTE, that is the question. The NLTE chemical evolution of strontium in extremely metal-poor stars. HANSEN C.J., BERGEMANN M., CESCUTTI G., et al.
2014ApJ...788..180C viz 16       D               1 329 52 Carbon-enhanced metal-poor stars: CEMP-s and CEMP-no subclasses in the halo system of the Milky Way. CAROLLO D., FREEMAN K., BEERS T.C., et al.
2016A&A...591A.118S viz 16       D               3 31406 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2017AJ....154...52M viz 16       D               1 68 12 High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. III. Unevolved stars with [Fe/H] <= -3.5. MATSUNO T., AOKI W., BEERS T.C., et al.
2020A&A...636A.115D 17       D               2 94 38 Reviving old controversies: is the early Galaxy flat or round?. Investigations into the early phases of the Milky Way's formation through stellar kinematics and chemical abundances. DI MATTEO P., SPITE M., HAYWOOD M., et al.

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