HE 0100-1622 , the SIMBAD biblio

HE 0100-1622 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:40:43


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Title First 3 Authors
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.
2015ApJ...807..173H 251       D     X         7 53 112 An elemental assay of very, extremely, and ultra-metal-poor stars. HANSEN T., HANSEN C.J., CHRISTLIEB N., et al.
2015A&A...580A..32M 94       D     X         3 48 13 The first stars: a classification of CEMP-no stars. MAEDER A. and MEYNET G.
2016MNRAS.456.1803F 22       D               1 11 145 s-process production in rotating massive stars at solar and low metallicities. FRISCHKNECHT U., HIRSCHI R., PIGNATARI M., 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.
2016ApJ...833...20Y viz 16       D               2 304 147 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.
2019A&A...623A.128H viz 16       D               1 100 36 Abundances and kinematics of carbon-enhanced metal-poor stars in the Galactic halo. A new classification scheme based on Sr and Ba. HANSEN C.J., HANSEN T.T., KOCH A., et al.
2019ApJ...879...37N 16       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.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
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.
2023A&A...679A..72M 17       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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