SDSS J220924.74-002859.8 , the SIMBAD biblio

SDSS J220924.74-002859.8 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST17:44:22


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Title First 3 Authors
2013A&A...552A.107S 675       D S   X C       16 9 131 Carbon-enhanced metal-poor stars: the most pristine objects? SPITE M., CAFFAU E., BONIFACIO P., et al.
2013AJ....146..132L 55       D     X         2 39 128 Carbon-enhanced metal-poor stars in SDSS/SEGUE. I. Carbon abundance estimation and frequency of CEMP stars. LEE Y.S., BEERS T.C., MASSERON T., et al.
2014ApJ...797...21P viz 93       D       C       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.
2015ApJ...809..136P 55       D     X         2 24 39 Metal-poor stars observed with the Magellan telescope. III. New extremely and ultra metal-poor stars from SDSS/SEGUE and insights on the formation of ultra metal-poor stars. PLACCO V.M., FREBEL A., LEE Y.S., 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.
2017MNRAS.468..418F 135       D     X   F     3 51 15 The mass distribution of Population III stars. FRASER M., CASEY A.R., GILMORE G., et al.
2017ApJ...847..142E viz 175       D     X         5 25 19 Ultra-metal-poor stars: spectroscopic determination of stellar atmospheric parameters using iron Non-LTE line abundances. EZZEDDINE R., FREBEL A. and PLEZ B.
2017A&A...605A..63C 56       D     X         2 24 5 Pre-supernova mixing in CEMP-no source stars. CHOPLIN A., EKSTROM S., MEYNET G., et al.
2019MNRAS.485.3527S 382       D     X C       9 19 ~ Ultra metal-poor stars: improved atmospheric parameters and NLTE abundances of magnesium and calcium. SITNOVA T.M., MASHONKINA L.I., EZZEDDINE R., et al.
2019MNRAS.486.5917K 81           X         2 12 ~ Effect of interstellar objects on metallicity of low-mass first stars formed in a cosmological model. KIRIHARA T., TANIKAWA A. and ISHIYAMA T.
2019ApJ...879...37N 97       D       C       3 74 7 The most metal-poor stars. V. The CEMP-no stars in 3D and non-LTE. NORRIS J.E. and YONG D.
2020ApJ...889L..13G 66     A     X         2 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.
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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