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| BPS BS 16929-0005 , the SIMBAD biblio (41 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST06:36:34 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2000AJ....120.1516A | 349 | 22 | The INT search for metal-poor stars: spectroscopic observations and classification via artificial neural networks. | ALLENDE PRIETO C., REBOLO R., GARCIA LOPEZ R.J., et al. | |||||
|
2004A&A...422..527S |
500 | 36 | uvby-β photometry of high-velocity and metal-poor stars. X. Stars of very low metal abundance: Observations, reddenings, metallicities, classifications, distances, and relative ages. | SCHUSTER W.J., BEERS T.C., MICHEL R., et al. | |||||
|
2004AJ....128.2402L |
135 | 16 | Abundances of extremely metal-poor star candidates. | LAI D.K., BOLTE M., JOHNSON J.A., et al. | |||||
| 2004ApJ...607..474H | 4 | 23 | 286 | Spectroscopic studies of extremely metal-poor stars with the Subaru High Dispersion Spectrograph. II. The r-process elements, including thorium. | HONDA S., AOKI W., KAJINO T., et al. | ||||
| 2004ApJS..152..113H | 22 | 39 | Spectroscopic studies of extremely metal-poor stars with the SUBARU high dispersion spectrograph. I. Observational data. | HONDA S., AOKI W., ANDO H., et al. | |||||
| 2004MmSAI..75..772T | 17 | 13 | On the binarity of carbon-enhanced, metal-poor stars. | TSANGARIDES S., RYAN S.G. and BEERS T.C. | |||||
|
2005AJ....130.2804R |
166 | 34 | Estimation of carbon abundances in metal-poor stars. I. Application to the strong G-band stars of Beers, Preston, and Shectman. | ROSSI S., BEERS T.C., SNEDEN C., et al. | |||||
|
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. | |||
|
2007ApJ...655..492A |
1 | 70 | 376 | Carbon-enhanced metal-poor stars. I. Chemical compositions of 26 stars. | AOKI W., BEERS T.C., CHRISTLIEB N., et al. | ||||
|
2007ApJ...658..367K |
15 | D | 1 | 122 | 103 | The origin of carbon enhancement and the initial mass function of extremely metal-poor stars in the Galactic halo. | KOMIYA Y., SUDA T., MINAGUCHI H., et al. | ||
|
2008ApJ...681.1524L |
91 | D | C | 11 | 60 | 270 | Detailed abundances for 28 metal-poor stars: stellar relics in the Milky Way. | LAI D.K., BOLTE M., JOHNSON J.A., et al. | |
|
2010A&A...509A..93M |
15 | D | 2 | 181 | 196 | A holistic approach to carbon-enhanced metal-poor stars. | MASSERON T., JOHNSON J.A., PLEZ B., et al. | ||
|
2010A&A...515A.111S |
15 | D | 1 | 17230 | 227 | The PASTEL catalogue of stellar parameters. | SOUBIRAN C., LE CAMPION J.-F., CAYREL DE STROBEL G., et al. | ||
| 2010A&A...524A..58T | 16 | D | 1 | 45 | 138 | Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans. | TAFELMEYER M., JABLONKA P., HILL V., et al. | ||
|
2011MNRAS.412..843S |
15 | D | 1 | 148 | 109 | The stellar abundances for galactic archaeology (SAGA) data base – II. Implications for mixing and nucleosynthesis in extremely metal-poor stars and chemical enrichment of the galaxy. | SUDA T., YAMADA S., KATSUTA Y., et al. | ||
|
2013ApJ...762...26Y |
15 | D | 1 | 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...27Y |
15 | D | 1 | 88 | 106 | 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. | ||
| 2013ApJ...762...28N | 15 | 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. | ||
|
2012A&A...548A..34A |
778 | D | X C | 20 | 134 | 38 | Elemental abundances and classification of carbon-enhanced metal-poor stars. | ALLEN D.M., RYAN S.G., ROSSI S., et al. | |
|
2013MNRAS.434.1681C |
15 | D | 1 | 91 | 74 | The near-infrared CaII triplet as a metallicity indicator - II. Extension to extremely metal-poor metallicity regimes. | CARRERA R., PANCINO E., GALLART C., et al. | ||
|
2014ApJ...788..180C |
15 | 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. | ||
| 2014MNRAS.441.1217S | 96 | D | F | 7 | 19 | 130 | Binarity in carbon-enhanced metal-poor stars. | STARKENBURG E., SHETRONE M.D., McCONNACHIE A.W., et al. | |
|
2014ApJ...797...21P |
15 | 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 | 55 | D | X | 2 | 44 | 35 | The first stars: CEMP-no stars and signatures of spinstars. | MAEDER A., MEYNET G. and CHIAPPINI C. | |
| 2015A&A...580A..32M | 94 | D | X | 3 | 48 | 13 | The first stars: a classification of CEMP-no stars. | MAEDER A. and MEYNET G. | |
| 2015ApJ...809..110C | 118 | X | 3 | 12 | 34 | Chemistry of the most metal-poor stars in the bulge and the z ≳ 10 universe. | CASEY A.R. and SCHLAUFMAN K.C. | ||
| 2016A&A...586A.160H | 95 | D | O C | 5 | 36 | 87 | The role of binaries in the enrichment of the early Galactic halo. II. Carbon-enhanced metal-poor stars: CEMP-no stars. | HANSEN T.T., ANDERSEN J., NORDSTROEM B., et al. | |
| 2016MNRAS.456.1803F | 22 | D | 1 | 11 | 145 | s-process production in rotating massive stars at solar and low metallicities. | FRISCHKNECHT U., HIRSCHI R., PIGNATARI M., et al. | ||
|
2016A&A...591A.118S |
16 | D | 1 | 31408 | 141 | The PASTEL catalogue: 2016 version. | SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., 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. | ||
|
2018ApJ...857...46I |
16 | D | 1 | 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. | ||
|
2019A&A...621A.108A |
301 | D | X | 8 | 59 | 49 | Binarity among CEMP-no stars: an indication of multiple formation pathways? | ARENTSEN A., STARKENBURG E., SHETRONE M.D., et al. | |
|
2019A&A...623A.128H |
16 | 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 | 122 | X 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. | ||
|
2021ApJ...908...79G |
42 | X | 1 | 46 | 33 | The r-process Alliance: chemodynamically tagged groups of halo r-process-enhanced stars reveal a shared chemical-evolution history. | GUDIN D., SHANK D., BEERS T.C., et al. | ||
|
2021ApJ...923..183L |
17 | D | 1 | 147 | ~ | Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. | LI H. | ||
|
2022A&A...663A...4S |
17 | D | 1 | 14206 | 7 | Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. | SOUBIRAN C., BROUILLET N. and CASAMIQUELA L. | ||
|
2023ApJ...947...23Z |
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. | ||
| 2023A&A...679A..72M | 17 | D | 1 | 56 | ~ | The 12C/13C isotopic ratio at the dawn of chemical evolution. | MOLARO P., AGUADO D.S., CAFFAU E., et al. | ||
| 2024ApJ...970L..30X | 18 | D | 1 | 81 | ~ | Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78. | XIE X.-J., SHI J., YAN H.-L., et al. | ||
| 2025ApJ...992..215I | 345 | D | X C | 7 | 21 | ~ | Potassium Abundances in Extremely Metal Poor Stars: Implications for Nucleosynthesis in the Final Stages of Massive Star Evolution. | ISHIGAKI M.N., TOMINAGA N., AOKI W., et al. |