BPS BS 16076-0006 , the SIMBAD biblio

BPS BS 16076-0006 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST14:09:04


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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.
2004AJ....128.2402L viz 135 16 Abundances of extremely metal-poor star candidates. LAI D.K., BOLTE M., JOHNSON J.A., 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.
2009A&A...501..519B viz 471       D     X C       12 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...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 43         O X         1 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.
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.
2013ApJ...762...27Y viz 16       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 16       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.
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...785...98T 135       D     X         4 55 110 Abundance profiling of extremely metal-poor stars and supernova properties in the early universe. TOMINAGA N., IWAMOTO N. and NOMOTO K.
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.
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 31406 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2017MNRAS.468..418F 97       D         F     2 51 15 The mass distribution of Population III stars. FRASER M., CASEY A.R., GILMORE G., 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 84             C       2 261 ~ Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars. CHOPLIN A., TOMINAGA N. and ISHIGAKI M.N.
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.
2021ApJ...907...10L viz 17       D               1 1549 37 Dynamically tagged groups of very metal-poor halo stars from the HK and Hamburg/ESO surveys. LIMBERG G., ROSSI S., BEERS T.C., et al.

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