HE 0049-3948 , the SIMBAD biblio

HE 0049-3948 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.09.23CEST18:01:58


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Title First 3 Authors
2019MNRAS.486.5917K 140           X         3 12 ~ Effect of interstellar objects on metallicity of low-mass first stars formed in a cosmological model. KIRIHARA T., TANIKAWA A. and ISHIYAMA T.
2018ApJ...857...46I viz 18       D               1 206 9 The initial mass function of the first stars inferred from extremely metal-poor stars. ISHIGAKI M.N., TOMINAGA N., KOBAYASHI C., et al.
2017A&A...605A..63C 192       D S     C       4 24 5 Pre-supernova mixing in CEMP-no source stars. CHOPLIN A., EKSTROM S., MEYNET G., et al.
2017MNRAS.468..418F 104       D         F     2 51 8 The mass distribution of Population III stars. FRASER M., CASEY A.R., GILMORE G., et al.
2016A&A...591A.118S viz 17       D               1 31387 40 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2014A&A...571A..62C 41           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...785...98T 141       D     X         4 55 66 Abundance profiling of extremely metal-poor stars and supernova properties in the early universe. TOMINAGA N., IWAMOTO N. and NOMOTO K.
2014ApJ...788..180C viz 16       D               1 329 37 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.
2013ApJ...762...25N viz 16       D               1 74 45 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               3 198 138 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...27Y viz 16       D               1 88 74 The most metal-poor stars. III. The metallicity distribution function and carbon-enhanced metal-poor fraction. YONG D., NORRIS J.E., BESSELL M.S., et al.
1995A&AS..112..347C viz 567 40 The ESO key-programme "A homogeneous bright QSO survey". I. The methods and the "deep" fields. CRISTIANI S., LA FRANCA F., ANDREANI P., et al.

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2020.09.23-18:01:58

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