other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
HE 1310-0536 , the SIMBAD biblio (30 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:55:47 |
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 |
---|---|---|---|---|---|---|---|---|---|
2007ApJS..168..128B | 15 | D | 1852 | 38 | Broadband UBVRCIC photometry of horizontal-branch and metal-poor candidates from the HK and Hamburg/ESO surveys. I. | BEERS T.C., FLYNN C., ROSSI S., et al. | |||
2014ApJ...787..162H | 490 | D | X C | 12 | 14 | 56 | Exploring the origin of lithium, carbon, strontium, and barium with four new ultra metal-poor stars. | HANSEN T., HANSEN C.J., CHRISTLIEB N., et al. | |
2014ApJ...791..116C | 81 | C | 1 | 13 | 64 | Carbon-enhanced metal-poor stars: relics from the dark ages. | COOKE R.J. and MADAU P. | ||
2014ApJ...797...21P | 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. | ||
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...579A..28B | 215 | D | X C | 5 | 46 | 146 | TOPoS. II. On the bimodality of carbon abundance in CEMP stars. Implications on the early chemical evolution of galaxies. | BONIFACIO P., CAFFAU E., SPITE M., 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. | |
2015ApJ...809..136P | 16 | D | 1 | 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. | ||
2015PASJ...67...84L | 931 | D | X C | 23 | 7 | 30 | High-resolution spectroscopic studies of ultra metal-poor stars found in the LAMOST survey. | LI H., AOKI W., ZHAO G., et al. | |
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 | 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. | ||
2016ApJ...833...21P | 58 | D | X | 2 | 13 | 33 | Observational constraints on first-star nucleosynthesis. II. Spectroscopy of an ultra metal-poor CEMP-no star. | PLACCO V.M., FREBEL A., BEERS T.C., et al. | |
2017MNRAS.468..418F | 97 | D | F | 2 | 51 | 15 | The mass distribution of Population III stars. | FRASER M., CASEY A.R., GILMORE G., et al. | |
2017ApJ...847..142E | 260 | D | X | 7 | 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. | |
2018MNRAS.474L..37C | 49 | X | 1 | 6 | 50 | Pop III i-process nucleosynthesis and the elemental abundances of SMSS J0313-6708 and the most iron-poor stars. | CLARKSON O., HERWIG F. and PIGNATARI M. | ||
2018ApJ...857...46I | 16 | D | 2 | 205 | 88 | The initial mass function of the first stars inferred from extremely metal-poor stars. | ISHIGAKI M.N., TOMINAGA N., KOBAYASHI C., et al. | ||
2019ApJ...871..146F | 17 | D | 1 | 33 | 17 | Chemical abundance signature of J0023+0307 a second-generation main-sequence star with [Fe/H] < -6. | FREBEL A., JI A.P., EZZEDDINE R., et al. | ||
2019MNRAS.484.2166S | 101 | D | F | 5 | 45 | 69 | Tracing the formation of the Milky Way through ultra metal-poor stars. | SESTITO F., LONGEARD N., MARTIN N.F., 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. | ||
2019MNRAS.485.3527S | 393 | 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. | |
2019ApJ...879...37N | 17 | D | 1 | 74 | 7 | The most metal-poor stars. V. The CEMP-no stars in 3D and non-LTE. | NORRIS J.E. and YONG D. | ||
2019MNRAS.489.5900D | 42 | X | 1 | 205 | 44 | The SkyMapper DR1.1 search for extremely metal-poor stars. | DA COSTA G.S., BESSELL M.S., MACKEY A.D., et al. | ||
2020ApJ...894....7Y | 187 | D | X C | 4 | 16 | ~ | Identification of a Group III CEMP-no star in the dwarf spheroidal galaxy Canes Venatici I. | YOON J., WHITTEN D.D., BEERS T.C., et al. | |
2020ApJ...894...34D | 17 | D | 1 | 24035 | ~ | The metallicity gradient and complex formation history of the outermost halo of the Milky Way. | DIETZ S.E., YOON J., BEERS T.C., et al. | ||
2021MNRAS.503.2539C | 17 | D | 1 | 479 | 34 | Exploring the Galaxy's halo and very metal-weak thick disc with SkyMapper and Gaia DR2. | CORDONI G., DA COSTA G.S., YONG D., et al. | ||
2023AJ....165...55C | 47 | X | 1 | 30 | 12 | Detailed Chemical Abundances of Stars in the Outskirts of the Tucana II Ultrafaint Dwarf Galaxy. | CHITI A., FREBEL A., JI A.P., et al. | ||
2023ApJ...947...23Z | 49 | X | 1 | 7 | 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. | ||
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. |