HE 2323-6549 , the SIMBAD biblio

HE 2323-6549 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:52:14

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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
1999ApJS..123..639N viz 2628 37 A search for stars of very low metal abundance. III. UBV photometry of metal-weak candidates. NORRIS J.E., RYAN S.G. and BEERS T.C.
2014ApJ...781...40P viz 635       D     X C       16 13 28 Metal-poor stars observed with the Magellan telescope. II. Discovery of four stars with [Fe/H] ≤ -3.5. PLACCO V.M., FREBEL A., BEERS T.C., et al.
2014ApJ...797...21P viz 15       D               2 606 226 Carbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundances. PLACCO V.M., FREBEL A., BEERS T.C., 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.
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.
2021ApJ...907...10L viz 17       D               1 1549 37 Dynamically tagged groups of very metal-poor halo stars from the HK and Hamburg/ESO surveys. LIMBERG G., ROSSI S., BEERS T.C., 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...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.

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