UCAC4 490-054409 , the SIMBAD biblio

UCAC4 490-054409 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST18:30:03

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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
2015RAA....15.1264L 2185 T   A D S   X C       54 3 10 Discovery of a strongly r-process enhanced extremely metal-poor star
LAMOST
J110901.22+075441.8. 		LI H.-N., AOKI W., HONDA S., et al.
2019ApJ...882...40J viz 16       D               1 210 41 The lanthanide fraction distribution in metal-poor stars: a test of neutron star mergers as the dominant r-process site. JI A.P., DROUT M.R. and HANSEN T.T.
2019A&A...632A..62C 81             C       1 261 ~ Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars. CHOPLIN A., TOMINAGA N. and ISHIGAKI M.N.
2020ApJ...894...34D viz 16       D               1 24035 ~ The metallicity gradient and complex formation history of the outermost halo of the Milky Way. DIETZ S.E., YOON J., BEERS T.C., et al.
2020ApJ...903...88M viz 3337 T   A D S   X C       79 6 22 Cosmological insights into the early accretion of r-process-enhanced stars. I. A comprehensive chemodynamical analysis of
LAMOST

J1109+0754. 		MARDINI M.K., PLACCO V.M., MEIRON Y., et al.
2021MNRAS.503.2539C viz 17       D               1 478 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.
2021ApJ...913...11L viz 17       D               1 1901 19 Targeting bright metal-poor stars in the disk and halo systems of the Galaxy. LIMBERG G., SANTUCCI R.M., ROSSI S., et al.
2021MNRAS.507.4102Y viz 100       D     X         3 162 16 High-resolution spectroscopic follow-up of the most metal-poor candidates from SkyMapper DR1.1. YONG D., DA COSTA G.S., BESSELL M.S., et al.
2021ApJ...923..183L viz 17       D               1 147 ~ Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. LI H.
2022ApJ...926...26S viz 17       D               1 6507 18 Dynamically Tagged Groups of Metal-poor Stars from the Best and Brightest Survey. SHANK D., BEERS T.C., PLACCO V.M., et al.
2022ApJ...931..146A viz 17       D               1 423 7 Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency. AOKI W., LI H., MATSUNO T., et al.
2022ApJ...931..147L viz 17       D               1 397 21 Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances. LI H., AOKI W., MATSUNO T., et al.
2023ApJ...943...23S viz 17       D               1 1792 5 The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars. SHANK D., BEERS T.C., PLACCO V.M., et al.
2023ApJ...946...48H viz 17       D               2 181 5 Finding r-II Sibling Stars in the Milky Way with the Greedy Optimistic Clustering Algorithm. HATTORI K., OKUNO A. and ROEDERER I.U.
2023RAA....23g5019S 17       D               1 95 ~ Sodium Abundances in Very Metal-poor Stars. SHEN Y.-F., ALEXEEVA S.A., ZHAO G., et al.
2023ApJ...959...60P 17       D               1 38 ~ SPLUS J142445.34-254247.1: An r-process-enhanced, Actinide-boost, Extremely Metal-poor Star Observed with GHOST. PLACCO V.M., ALMEIDA-FERNANDES F., HOLMBECK E.M., et al.
2024ApJ...970L..30X 18       D               1 81 ~ Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78. XIE X.-J., SHI J., YAN H.-L., et al.
2025ApJ...995..165J 19       D               4 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.
2026ApJ...998..139A 20       D               1 104 ~ A Systematic NLTE Study of Very Metal-poor Stars with Metallicity down to -4.3 dex. VI. Light Neutron-capture Elements and the Sr-Na Correlation as a Signature of Spinstar Nucleosynthesis in the Early Galaxy. ALEXEEVA S., YAN H., ZHAO G., et al.

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