HE 2139-5432 , the SIMBAD biblio

HE 2139-5432 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST16:18:11


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Title First 3 Authors
2013ApJ...762...25N viz 16       D               1 74 50 The most metal-poor stars. I. Discovery, data, and atmospheric parameters. NORRIS J.E., BESSELL M.S., YONG D., et al.
2013ApJ...762...26Y viz 250       D     X         7 198 263 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               3 106 171 The most metal-poor stars. IV. The two populations with [Fe/H] ≲ -3.0. NORRIS J.E., YONG D., BESSELL M.S., et al.
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...791..116C 81             C       1 13 64 Carbon-enhanced metal-poor stars: relics from the dark ages. COOKE R.J. and MADAU P.
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.
2015A&A...576A..56M 16       D               1 44 35 The first stars: CEMP-no stars and signatures of spinstars. MAEDER A., MEYNET G. and CHIAPPINI C.
2015A&A...580A..32M 56       D     X         2 48 13 The first stars: a classification of CEMP-no stars. MAEDER A. and MEYNET G.
2015ApJ...809..136P 16       D               1 24 39 Metal-poor stars observed with the Magellan telescope. III. New extremely and ultra metal-poor stars from SDSS/SEGUE and insights on the formation of ultra metal-poor stars. PLACCO V.M., FREBEL A., LEE Y.S., et al.
2016A&A...591A.118S viz 16       D               1 31406 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2016ApJ...833...20Y viz 96       D     X         3 304 147 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.
2016ApJ...833...21P 98       D     X         3 13 33 Observational constraints on first-star nucleosynthesis. II. Spectroscopy of an ultra metal-poor CEMP-no star. PLACCO V.M., FREBEL A., BEERS T.C., 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.
2017ApJ...847..142E viz 422       D     X         11 25 19 Ultra-metal-poor stars: spectroscopic determination of stellar atmospheric parameters using iron Non-LTE line abundances. EZZEDDINE R., FREBEL A. and PLEZ B.
2017A&A...605A..63C 260       D S   X C       5 24 5 Pre-supernova mixing in CEMP-no source stars. CHOPLIN A., EKSTROM S., MEYNET G., et al.
2018ApJ...857...46I viz 16       D               2 205 88 The initial mass function of the first stars inferred from extremely metal-poor stars. ISHIGAKI M.N., TOMINAGA N., KOBAYASHI C., et al.
2018A&A...611A..30S 41           X         1 21 14 Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars. SPITE F., SPITE M., BARBUY B., et al.
2019A&A...621A.108A viz 476       D     X C       11 59 49 Binarity among CEMP-no stars: an indication of multiple formation pathways? ARENTSEN A., STARKENBURG E., SHETRONE M.D., et al.
2019ApJ...871..146F 17       D               1 33 17 Chemical abundance signature of J0023+0307 a second-generation main-sequence star with [Fe/H] < -6. FREBEL A., JI A.P., EZZEDDINE R., et al.
2018PASJ...70...94A 141       D     X         4 7 8 LAMOST J221750.59+210437.2: A new member of carbon-enhanced extremely metal-poor stars with excesses of Mg and Si. AOKI W., MATSUNO T., HONDA S., et al.
2019MNRAS.484.2166S 101       D         F     5 45 69 Tracing the formation of the Milky Way through ultra metal-poor stars. SESTITO F., LONGEARD N., MARTIN N.F., et al.
2019MNRAS.485.3527S 602       D     X         15 19 ~ Ultra metal-poor stars: improved atmospheric parameters and NLTE abundances of magnesium and calcium. SITNOVA T.M., MASHONKINA L.I., EZZEDDINE R., et al.
2019ApJ...879...37N 17       D               1 74 7 The most metal-poor stars. V. The CEMP-no stars in 3D and non-LTE. NORRIS J.E. and YONG D.
2019MNRAS.489.5900D viz 226       D     X         6 205 44 The SkyMapper DR1.1 search for extremely metal-poor stars. DA COSTA G.S., BESSELL M.S., MACKEY A.D., et al.
2020ApJ...901..105Z 43           X         1 6 ~ A carbon-enhanced Lyman limit system: signature of the first generation of stars? ZOU S., PETITJEAN P., NOTERDAEME P., et al.
2021MNRAS.503.2539C viz 17       D               1 479 34 Exploring the Galaxy's halo and very metal-weak thick disc with SkyMapper and Gaia DR2. CORDONI G., DA COSTA G.S., YONG D., et al.
2021ApJS..254...31C viz 94           X         2 3 22 Stellar metallicities from SkyMapper photometry. II. Precise photometric metallicities of ∼280,000 giant stars with [Fe/H] < -0.75 in the Milky Way. CHITI A., FREBEL A., MARDINI M.K., et al.
2023MNRAS.518.4557S 47           X         1 35 9 The Pristine Inner Galaxy Survey (PIGS) - V. A chemo-dynamical investigation of the early assembly of the Milky Way with the most metal-poor stars in the bulge. SESTITO F., VENN K.A., ARENTSEN A., et al.
2023MNRAS.525.1311P 439       D     X   F     9 38 ~ Field blue straggler stars: discovery of white dwarf companions to blue metal-poor stars using UVIT/AstroSat. PANTHI A., SUBRAMANIAM A., VAIDYA K., et al.
2023A&A...679A..72M 19       D               1 56 ~ The 12C/13C isotopic ratio at the dawn of chemical evolution. MOLARO P., AGUADO D.S., CAFFAU E., et al.

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