UCAC4 556-136576 , the SIMBAD biblio

UCAC4 556-136576 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST10:41:57

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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
2019ApJ...871..146F 81           X         2 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 1085 T   A D     X C       26 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.
2019A&A...632A..62C 122           X 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.
2020ApJ...889L..13G 41           X         1 10 ~ The extreme CNO-enhanced composition of the primitive iron-poor dwarf star J0815+4729. GONZALEZ HERNANDEZ J.I., AGUADO D.S., ALLENDE PRIETO C., et al.
2021ApJ...923..183L viz 17       D               1 147 ~ Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. LI H.
2022PASJ...74..273A 613       D     X         15 7 2 Silicon and strontium abundances of very metal-poor stars determined from near-infrared spectra. AOKI W., BEERS T.C., HONDA S., 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.
2023RAA....23g5019S 17       D               1 95 ~ Sodium Abundances in Very Metal-poor Stars. SHEN Y.-F., ALEXEEVA S.A., ZHAO G., et al.
2024ApJ...966..174Z 134           X         3 19 ~ Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties. ZHANG R., MATSUNO T., LI H., et al.
2024ApJS..274...39B viz 376       D     X         9 42 ~ The R-process Alliance: Fifth Data Release from the Search for R-process-enhanced Metal-poor Stars in the Galactic Halo with the GTC. BANDYOPADHYAY A., EZZEDDINE R., ALLENDE PRIETO C., et al.
2025MNRAS.540..331H 187             C F     2 10 ~ Formation of first star clusters under the supersonic gas flow - II. Critical halo mass and core mass function. HIRANO S.
2025PASJ...77..502A 672       D     X C       14 46 ~ Elemental abundances of 44 very metal-poor stars determined from Subaru/IRD near-infrared spectra. AOKI W., BEERS T.C., HONDA S., 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 270       D     X         6 104 ~ 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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