HE 0450-4902 , the SIMBAD biblio

HE 0450-4902 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST11:47:33

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2015ApJ...807..173H 212       D     X         6 53 112 An elemental assay of very, extremely, and ultra-metal-poor stars. HANSEN T., HANSEN C.J., CHRISTLIEB N., 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               1 304 147 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.
2019A&A...632A..62C 81             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...634A..72S 16       D               1 83 ~ An empirical metallicity tracer in CEMP and C-normal stars. SINGH D., HANSEN C.J., BYRGESEN J.S., et al.
2021A&A...645A..10G viz 42         O X         1 10 ~ Nucleosynthetic yields of Z = 10–5 intermediate-mass stars. GIL-PONS P., DOHERTY C.L., GUTIERREZ J., et al.
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.
2025A&A...704A.103S viz 299       D     X         7 10 ~ Distinct barium isotope ratios in CEMP-s and CEMP-rs stars. SITNOVA T.M., MASHONKINA L.I., ROMANOVSKAYA A.M., et al.

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