HE 0228-4047 , the SIMBAD biblio

HE 0228-4047 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:56:57


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Title First 3 Authors
2013ApJ...762...25N viz 15       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 15       D               6 198 263 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               2 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.
2014ApJ...785...98T 133       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 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.
2014A&A...571A..62C 39           X         1 44 3 Chemical abundances of the metal-poor horizontal-branch stars BPS CS 22186-005. CALISKAN S., CAFFAU E., BONIFACIO P., et al.
2016A&A...591A.118S viz 16       D               2 31408 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2017A&A...605A..63C 16       D               1 24 5 Pre-supernova mixing in CEMP-no source stars. CHOPLIN A., EKSTROM S., MEYNET G., et al.
2019MNRAS.486.5917K 122           X         3 12 ~ Effect of interstellar objects on metallicity of low-mass first stars formed in a cosmological model. KIRIHARA T., TANIKAWA A. and ISHIYAMA T.
2024A&A...691A.284R viz 18       D               1 80 ~ The earliest phases of CNO enrichment in galaxies. ROSSI M., ROMANO D., MUCCIARELLI A., et al.
2025ApJ...995..165J 19       D               1 76 ~ Abundance Pattern Fitting with Bayesian Inference: Constraining First Stars' Properties and Their Explosion Mechanism with Extremely Metal-poor Stars. JIANG R., LI H., ZHAO G., et al.

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