HE 2247-7400 , the SIMBAD biblio

HE 2247-7400 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST09:35:20


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Title First 3 Authors
2013ApJ...762...25N viz 16       D               1 74 50 The most metal-poor stars. I. Discovery, data, and atmospheric parameters. NORRIS J.E., BESSELL M.S., YONG D., et al.
2013ApJ...762...26Y viz 16       D               3 198 263 The most metal-poor stars. II. Chemical abundances of 190 metal-poor stars including 10 new stars with [Fe/H] ≤ -3.5. YONG D., NORRIS J.E., BESSELL M.S., et al.
2013ApJ...762...28N 16       D               3 106 171 The most metal-poor stars. IV. The two populations with [Fe/H] ≲ -3.0. NORRIS J.E., YONG D., BESSELL M.S., et al.
2014ApJ...788..180C viz 16       D               1 329 52 Carbon-enhanced metal-poor stars: CEMP-s and CEMP-no subclasses in the halo system of the Milky Way. CAROLLO D., FREEMAN K., BEERS T.C., et al.
2014A&A...571A..62C 39           X         1 44 3 Chemical abundances of the metal-poor horizontal-branch stars BPS CS 22186-005. CALISKAN S., CAFFAU E., BONIFACIO P., et al.
2014ApJ...797...21P viz 16       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.
2015A&A...576A..56M 16       D               1 44 35 The first stars: CEMP-no stars and signatures of spinstars. MAEDER A., MEYNET G. and CHIAPPINI C.
2015A&A...580A..32M 56       D     X         2 48 13 The first stars: a classification of CEMP-no stars. MAEDER A. and MEYNET G.
2016MNRAS.460..884H viz 83             C       1 24 76 The EMBLA survey - metal-poor stars in the Galactic bulge. HOWES L.M., ASPLUND M., KELLER S.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.
2019A&A...621A.108A viz 184       D     X         5 59 49 Binarity among CEMP-no stars: an indication of multiple formation pathways? ARENTSEN A., STARKENBURG E., SHETRONE M.D., et al.
2023A&A...679A..72M 19       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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