BPS BS 16077-0007 , the SIMBAD biblio

BPS BS 16077-0007 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:17:38

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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
2000AJ....119.2882A 529 23 A search for stars of very low metal abundance. IV. uvbyCa observations of metal-weak candidates from the northern HK survey. ANTHONY-TWAROG B.J., SARAJEDINI A., TWAROG B.A., et al.
2000AJ....120.2065B 268 117 A search for stars of very low metal abundance. V. Photoelectric UBV photometry of metal-weak candidates from the northern HK survey. BONIFACIO P., MONAI S. and BEERS T.C.
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....128.2402L viz 135 16 Abundances of extremely metal-poor star candidates. LAI D.K., BOLTE M., JOHNSON J.A., et al.
2008ApJ...681.1524L viz 17       D               10 60 270 Detailed abundances for 28 metal-poor stars: stellar relics in the Milky Way. LAI D.K., BOLTE M., JOHNSON J.A., et al.
2009AJ....137..272R viz 15       D               1 737 45 Chemical inhomogeneities in the Milky Way stellar halo. ROEDERER I.U.
2010A&A...515A.111S viz 15       D               1 17230 227 The PASTEL catalogue of stellar parameters. SOUBIRAN C., LE CAMPION J.-F., CAYREL DE STROBEL G., et al.
2011MNRAS.412..843S viz 15       D               1 148 109 The stellar abundances for galactic archaeology (SAGA) data base – II. Implications for mixing and nucleosynthesis in extremely metal-poor stars and chemical enrichment of the galaxy. SUDA T., YAMADA S., KATSUTA Y., et al.
2013ApJ...762...26Y viz 15       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.
2014ApJ...788..180C viz 15       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.
2014ApJ...797...21P viz 15       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               1 31408 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2021ApJ...923..183L viz 17       D               1 147 ~ Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. LI H.
2022ApJ...931..146A viz 17       D               1 423 7 Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency. AOKI W., LI H., MATSUNO T., et al.
2022ApJ...931..147L viz 17       D               1 397 21 Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances. LI H., AOKI W., MATSUNO T., et al.
2023ApJ...947...23Z viz 17       D               1 647 14 Chemodynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-s and CEMP-no Stars. ZEPEDA J., BEERS T.C., PLACCO V.M., et al.
2023RAA....23g5019S 17       D               1 95 ~ Sodium Abundances in Very Metal-poor Stars. SHEN Y.-F., ALEXEEVA S.A., ZHAO G., et al.
2025ApJ...983..127S 112       D     X         3 29 ~ A Systematic NLTE Study of Very Metal-poor Stars with Metallicity down to -4.3 dex. I. Global Stellar Parameters Based on High-resolution Spectra. SHI J., ZHAO G., LIU S., et al.
2026ApJ...998..139A 170       D     X C       3 104 ~ A Systematic NLTE Study of Very Metal-poor Stars with Metallicity down to -4.3 dex. VI. Light Neutron-capture Elements and the Sr-Na Correlation as a Signature of Spinstar Nucleosynthesis in the Early Galaxy. ALEXEEVA S., YAN H., ZHAO G., et al.

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