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HE 2331-7155 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST05:31:02 |
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 |
---|---|---|---|---|---|---|---|---|---|
2015ApJ...807..173H | 295 | D | X | 8 | 53 | 112 | An elemental assay of very, extremely, and ultra-metal-poor stars. | HANSEN T., HANSEN C.J., CHRISTLIEB N., et al. | |
2015A&A...580A..32M | 56 | D | X | 2 | 48 | 13 | The first stars: a classification of CEMP-no stars. | MAEDER A. and MEYNET G. | |
2016A&A...591A.118S | 16 | D | 1 | 31406 | 141 | The PASTEL catalogue: 2016 version. | SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al. | ||
2016A&A...593A..36C | 16 | D | 1 | 14 | 5 | Constraints on CEMP-no progenitors from nuclear astrophysics. | CHOPLIN A., MAEDER A., MEYNET G., et al. | ||
2016ApJ...833...20Y | 96 | D | C | 3 | 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. | |
2017A&A...605A..63C | 422 | D | S X C | 9 | 24 | 5 | Pre-supernova mixing in CEMP-no source stars. | CHOPLIN A., EKSTROM S., MEYNET G., et al. | |
2019A&A...623A.128H | 17 | D | 1 | 100 | 36 | Abundances and kinematics of carbon-enhanced metal-poor stars in the Galactic halo. A new classification scheme based on Sr and Ba. | HANSEN C.J., HANSEN T.T., KOCH A., et al. | ||
2019A&A...632A..62C | 84 | 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. | ||
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. | ||
2024ApJS..270...28R | 20 | D | 1 | 54 | ~ | Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei. | ROBERTI L., LIMONGI M. and CHIEFFI A. |