BPS CS 22949-0048 , the SIMBAD biblio

BPS CS 22949-0048 , the SIMBAD biblio (35 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.14CEST14:26:54

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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
1991ApJS...76.1001P viz 1762 52 Photoelectric UBV photometry of stars selected in the HK objective-prism survey. PRESTON G.W., SHECTMAN S.A. and BEERS T.C.
1992AJ....103.1987B viz 1024 532 A search for stars of very low metal abundance. II. BEERS T.C., PRESTON G.W. and SHECTMAN S.A.
1995AJ....109.2736M 1 33 163 A spectroscopic analysis of 33 of the most metal-poor stars. I. McWILLIAM A., PRESTON G.W., SNEDEN C., et al.
1995AJ....109.2757M 5 34 787 Spectroscopic analysis of 33 of the most metal-poor stars. II. McWILLIAM A., PRESTON G.W., SNEDEN C., et al.
1995ApJS...96..175B viz 1810 175 Kinematics of metal-poor stars in the Galaxy. BEERS T.C. and SOMMER-LARSEN J.
1996A&ARv...7..217C 35 32 The first generation of stars. CAYREL R.
1997A&AS..124..299C viz 3159 203 A catalogue of [Fe/H] determinations: 1996 edition. CAYREL DE STROBEL G., SOUBIRAN C., FRIEL E.D., et al.
1998AJ....115.1640M 3 34 400 Barium abundances in extremely metal-poor stars. McWILLIAM A.
1999AJ....117..981B viz 547 146 Estimation of stellar metal abundance. II. A recalibration of the Ca II K technique, and the autocorrelation function method. BEERS T.C., ROSSI S., NORRIS J.E., et al.
2000A&A...360.1077S 11 18 Element abundance ratios in an extremely metal-poor binary star: CS 22873-139. SPITE M., DEPAGNE E., NORDSTROEM B., et al.
2000AJ....119.2866B viz 2011 171 Kinematics of metal-poor stars in the Galaxy. II. Proper motions for a large nonkinematically selected sample. BEERS T.C., CHIBA M., YOSHII Y., et al.
2001A&A...373..159C viz 15       D               3320 239 Catalogue of [Fe/H] determinations for FGK stars: 2001 edition. CAYREL DE STROBEL G., SOUBIRAN C. and RALITE N.
2001ApJ...562..528S viz 280 35 Three-dimensional spectral classification of low-metallicity stars using artificial neural networks. SNIDER S., ALLENDE PRIETO C., VON HIPPEL T., et al.
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.
2004AJ....128.1177V viz 796 690 Stellar chemical signatures and hierarchical galaxy formation. VENN K.A., IRWIN M., SHETRONE M.D., et al.
2004AJ....128.2402L viz 135 16 Abundances of extremely metal-poor star candidates. LAI D.K., BOLTE M., JOHNSON J.A., et al.
2005AJ....130.2804R viz 166 34 Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. ROSSI S., BEERS T.C., SNEDEN C., et al.
2006AN....327...72B 359 19 Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes. BILIR S., KARAALI S., GUVER T., 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.
2011A&A...528A...9S 92       D     X         3 55 39 First stars. XIV. Sulfur abundances in extremely metal-poor stars. SPITE M., CAFFAU E., ANDRIEVSKY S.M., et al.
2011A&A...530A.105A 15       D               1 60 49 NLTE strontium abundance in a sample of extremely metal poor stars and the Sr/Ba ratio in the early Galaxy. ANDRIEVSKY S.M., SPITE F., KOROTIN S.A., et al.
2013AJ....145...26R 40           X         1 27 57 Are there any stars lacking neutron-capture elements? Evidence from strontium and barium. ROEDERER I.U.
2014AJ....147..136R viz 16       D               3 317 336 A search for stars of very low metal abundance. VI. Detailed abundances of 313 metal-poor stars. ROEDERER I.U., PRESTON G.W., THOMPSON I.B., et al.
2014ApJ...797...13S viz 16       D               2 518 84 The best and brightest metal-poor stars. SCHLAUFMAN K.C. and CASEY A.R.
2014ApJ...797...21P viz 16       D               2 606 226 Carbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundances. PLACCO V.M., FREBEL A., BEERS T.C., et al.
2016A&A...591A.118S viz 16       D               2 31407 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2016ApJ...833...20Y viz 16       D               2 304 147 Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. YOON J., BEERS T.C., PLACCO V.M., et al.
2018ApJ...857...46I viz 16       D               1 205 88 The initial mass function of the first stars inferred from extremely metal-poor stars. ISHIGAKI M.N., TOMINAGA N., KOBAYASHI C., et al.
2018ApJ...857..111T viz 17       D               1 73 76 Stellar yields of rotating first stars. II. Pair-instability supernovae and comparison with observations. TAKAHASHI K., YOSHIDA T. and UMEDA H.
2019A&A...632A..62C 84             C       1 261 ~ Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars. CHOPLIN A., TOMINAGA N. and ISHIGAKI M.N.
2020ApJ...900..106O viz 17       D               1 314 ~ Vanadium abundance derivations in 255 metal-poor stars. OU X., ROEDERER I.U., SNEDEN C., et al.
2022ApJ...926...26S viz 18       D               1 6455 18 Dynamically Tagged Groups of Metal-poor Stars from the Best and Brightest Survey. SHANK D., BEERS T.C., PLACCO V.M., et al.
2022A&A...663A...4S viz 18       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2023A&A...679A.110G viz 159       D     X         4 52 ~ TITANS metal-poor reference stars II. Red giants and CEMP stars. GIRIBALDI R.E., VAN ECK S., MERLE T., et al.
2024ApJS..270...28R 20       D               1 54 ~ Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei. ROBERTI L., LIMONGI M. and CHIEFFI A.

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