BPS BS 16920-0017 , the SIMBAD biblio

BPS BS 16920-0017 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:43:01


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Title First 3 Authors
2000AJ....120.1516A 349 22 The INT search for metal-poor stars: spectroscopic observations and classification via artificial neural networks. ALLENDE PRIETO C., REBOLO R., GARCIA LOPEZ R.J., 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.
2004ApJ...607..474H 4 23 286 Spectroscopic studies of extremely metal-poor stars with the Subaru High Dispersion Spectrograph. II. The r-process elements, including thorium. HONDA S., AOKI W., KAJINO T., et al.
2004ApJS..152..113H 22 39 Spectroscopic studies of extremely metal-poor stars with the SUBARU high dispersion spectrograph. I. Observational data. HONDA S., AOKI W., ANDO H., 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.
2008ApJ...681.1524L viz 17       D               1 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.
2011ApJ...730...77H 2425 T K A D     X C       63 26 9 Spectroscopic studies of extremely metal-poor stars with the Subaru high dispersion spectrograph. V. The zn-enhanced metal-poor star
BS 16920-017.
HONDA S., AOKI W., BEERS T.C., 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.
2013ApJ...762...27Y viz 15       D               1 88 106 The most metal-poor stars. III. The metallicity distribution function and carbon-enhanced metal-poor fraction. YONG D., NORRIS J.E., BESSELL M.S., et al.
2013ApJ...762...28N 15       D               1 106 171 The most metal-poor stars. IV. The two populations with [Fe/H] ≲ -3.0. NORRIS J.E., YONG D., BESSELL M.S., et al.
2013ApJ...778...56C viz 38           X         1 135 157 Normal and outlying populations of the Milky Way stellar halo at [Fe/H] ←2. COHEN J.G., CHRISTLIEB N., THOMPSON I., 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.
2016A&A...595L...6C 79             C       1 10 12 TOPoS. III. An ultra iron-poor multiple CEMP system. CAFFAU E., BONIFACIO P., SPITE 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.
2019A&A...632A..62C 162           X C       3 261 ~ Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars. CHOPLIN A., TOMINAGA N. and ISHIGAKI M.N.
2021A&A...651A..57N 293           X C       6 20 ~ G 112-43/44: A metal-poor binary star with a unique chemical composition and Helmi stream kinematics. NISSEN P.E., SILVA-CABRERA J.S. and SCHUSTER W.J.
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.
2025A&A...695A.112V viz 19       D               1 212 ~ The Pristine survey XXV. The very metal-poor Galaxy: Chemodynamics through the follow-up of the Pristine-Gaia synthetic catalogue. VISWANATHAN A., YUAN Z., ARDERN-ARENTSEN A., et al.

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