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BPS CS 29526-0110 , the SIMBAD biblio (51 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.09.27CEST13:04:12 |
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 |
---|---|---|---|---|---|---|---|---|---|
1999ApJS..123..639N ![]() |
2628 | 37 | A search for stars of very low metal abundance. III. UBV photometry of metal-weak candidates. | NORRIS J.E., RYAN S.G. and BEERS T.C. | |||||
2002ApJ...580.1149A | 7 | 8 | 180 | A Subaru/High dispersion spectrograph study of lead (Pb) abundances in eight s-process element-rich, metal-poor stars. | AOKI W., RYAN S.G., NORRIS J.E., et al. | ||||
2002PASJ...54..933A | 1 | 13 | 40 | Subaru/HDS study of extremely metal-poor star CS 29498-043 : abundance analysis details and comparison with other carbon-rich objects. | AOKI W., NORRIS J.E., RYAN S.G., et al. | ||||
2003A&A...404..291V | 2 | 14 | 108 | More lead stars. | VAN ECK S., GORIELY S., JORISSEN A., et al. | ||||
2003AJ....125..875L | 1 | 23 | 104 | Stellar archaeology: a Keck pilot program on extremely metal-poor stars from the Hamburg/ESO survey. III. The lead (Pb) star HE 0024-2523. | LUCATELLO S., GRATTON R., COHEN J.G., et al. | ||||
2003ApJ...588.1082C | 2 | 13 | 102 | Abundance analysis of HE 2148-1247, a star with extremely enhanced neutron capture elements. | COHEN J.G., CHRISTLIEB N., QIAN Y.-Z., et al. | ||||
2004A&A...413.1073S | 1 | 31 | 96 | First stars. IV. CS 29497-030: Evidence for operation of the s-process at very low metallicity. | SIVARANI T., BONIFACIO P., MOLARO P., 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. | |||||
2004MmSAI..75..706D | 14 | 10 | Lead and s-process elements in stars of various metallicities: AGB predictions compared with observation. | DELAUDE D., GALLINO R., CRISTALLO S., 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. | |||||
2005A&A...429.1031B | 3 | 11 | 84 | New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34: Binarity and neutron capture elements. | BARBUY B., SPITE M., SPITE F., et al. | ||||
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. | |||||
2005ApJ...625..825L | 5 | 23 | 265 | The binary frequency among carbon-enhanced, s-process-rich, metal-poor stars. | LUCATELLO S., TSANGARIDES S., BEERS T.C., et al. | ||||
2006A&A...451..651J | 1 | 44 | 134 | The Hamburg/ESO R-process enhanced star survey (HERES). III. HE 0338-3945 and the formation of the r + s stars. | JONSELL K., BARKLEM P.S., GUSTAFSSON B., et al. | ||||
2006ApJ...636..842W | 1 | 11 | 23 | Enrichment of very metal poor stars with both R-process and S-process elements from 8-10 M☉stars. | WANAJO S., NOMOTO K., IWAMOTO N., et al. | ||||
2006ApJ...642.1075Z | 15 | 20 | Neutron-capture elements in the s- and r-process-rich stars: constraints on neutron-capture nucleosynthesis processes. | ZHANG B., MA K. and ZHOU G. | |||||
2006A&A...459..125S | 1 | 28 | 64 | First stars X. The nature of three unevolved carbon-enhanced metal-poor stars. | SIVARANI T., BEERS T.C., BONIFACIO P., 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 ![]() |
2 | 70 | 376 | Carbon-enhanced metal-poor stars. I. Chemical compositions of 26 stars. | AOKI W., BEERS T.C., CHRISTLIEB N., et al. | ||||
2006MmSAI..77..985B | 33 | 10 | s-Process in low metallicity Pb stars. | BISTERZO S., GALLINO R., STRANIERO O., et al. | |||||
2007MNRAS.375.1418M | 17 | 3 | Investigation of the single neutron exposure model for the s-process: the primary nature of the neutron source. | MA K., CUI W. and ZHANG B. | |||||
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. | ||
2007ApJ...658.1203J ![]() |
15 | D | 69 | 54 | A search for nitrogen-enhanced metal-poor stars. | JOHNSON J.A., HERWIG F., BEERS T.C., et al. | |||
2008ApJ...678.1351A | 812 | D | X C | 21 | 27 | 106 | Carbon-enhanced metal-poor stars. III. Main-sequence turnoff stars from the SDSS SEGUE sample. | AOKI W., BEERS T.C., SIVARANI T., et al. | |
2008ApJ...679.1549R ![]() |
53 | D | X | 2 | 28 | 35 | The Hobby-Eberly telescope Chemical Abundances of Stars in the Halo (CASH) project. I. The lithium-, s-, and r-enhanced metal-poor giant HKII 17435-00532. | ROEDERER I.U., FREBEL A., SHETRONE M.D., et al. | |
2009ApJ...698.1963R | 38 | X | 1 | 57 | 66 | The end of nucleosynthesis: production of lead and thorium in the early galaxy. | ROEDERER I.U., KRATZ K.-L., FREBEL A., et al. | ||
2009PASA...26..314B | 2 | 5 | 20 | Interpretation of CEMP(s) and CEMP(s + r) stars with AGB models. | BISTERZO S., GALLINO R., STRANIERO O., 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. | ||
2010MNRAS.403..505S | 57 | D | X | 2 | 9 | 59 | The effects of thermohaline mixing on low-metallicity asymptotic giant branch stars. | STANCLIFFE R.J. | |
2010MNRAS.404..253G ![]() |
38 | X | 1 | 19 | 21 | HD209621: abundances of neutron-capture elements. | GOSWAMI A. and AOKI W. | ||
2010ApJ...724..975R ![]() |
38 | X | 1 | 197 | 141 | The ubiquity of the rapid neutron-capture process. | ROEDERER I.U., COWAN J.J., KARAKAS A.I., 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. | ||
2011MNRAS.418..284B ![]() |
15 | D | 3 | 115 | 191 | The s-process in low-metallicity stars – II. Interpretation of high-resolution spectroscopic observations with asymptotic giant branch models. | BISTERZO S., GALLINO R., STRANIERO O., et al. | ||
2012ApJ...751...14M | 16 | D | 1 | 50 | 38 | Lithium abundances in carbon-enhanced metal-poor stars. | MASSERON T., JOHNSON J.A., LUCATELLO S., et al. | ||
2012MNRAS.422..849B | 367 | D | S X C F | 7 | 97 | 85 | The s-process in low-metallicity stars - III. Individual analysis of CEMP-s and CEMP-s/r with asymptotic giant branch models. | BISTERZO S., GALLINO R., STRANIERO O., et al. | |
2013AJ....145...13A ![]() |
39 | X | 1 | 151 | 146 | High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. I. Atmospheric parameters and chemical compositions. | AOKI W., BEERS T.C., LEE Y.S., et al. | ||
2012A&A...548A..34A ![]() |
796 | 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. | |
2012PASP..124..304L | 16 | D | 1 | 34 | 2 | Abundance analysis of r + s stars: r -process abundance comparison between r + s stars and r rich stars. | LIANG S., LI H., SHEN S., et al. | ||
2013ApJ...770..104P | 16 | D | 1 | 33 | 40 | Metal-poor stars observed with the Magellan telescope. I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis. | PLACCO V.M., FREBEL A., BEERS T.C., et al. | ||
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. | ||
2015A&A...581A..22A ![]() |
16 | D | 4 | 66 | 34 | Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution. II. Statistical analysis of a sample of 67 CEMP-s stars. | ABATE C., POLS O.R., IZZARD R.G., et al. | ||
2015ApJ...814..121H ![]() |
16 | D | 1 | 26 | 9 | The Chemical Abundances of Stars in the Halo (CASH) Project. III. A new classification scheme for carbon-enhanced metal-poor stars with s-process element enhancement. | HOLLEK J.K., FREBEL A., PLACCO V.M., et al. | ||
2016A&A...593A..62M | 41 | X | 1 | 13 | 2 | The odd-isotope fractions of barium in CEMP-r/s star HE 0338-3945 and r-II star CS 31082-001. | MENG X.Y., CUI W.Y., SHI J.R., et al. | ||
2016ApJ...831..171H | 102 | D | C | 3 | 23 | 126 | The intermediate neutron-capture process and carbon-enhanced metal-poor stars. | HAMPEL M., STANCLIFFE R.J., LUGARO M., et al. | |
2016ApJ...833...20Y ![]() |
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. | ||
2019ApJ...887...11H | 17 | D | 2 | 34 | ~ | Learning about the intermediate neutron-capture process from lead abundances. | HAMPEL M., KARAKAS A.I., STANCLIFFE R.J., et al. | ||
2020ApJ...891...39Y ![]() |
20 | D | 1 | 30 | 92 | Dynamical relics of the ancient galactic halo. | YUAN Z., MYEONG G.C., BEERS T.C., et al. | ||
2021ApJ...907...10L ![]() |
18 | D | 1 | 1549 | 37 | Dynamically tagged groups of very metal-poor halo stars from the HK and Hamburg/ESO surveys. | LIMBERG G., ROSSI S., BEERS T.C., et al. | ||
2021ApJ...908...79G ![]() |
45 | 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. | ||
2021A&A...649A..49G ![]() |
18 | D | 1 | 87 | 17 | Spectroscopic study of CEMP-(s & r/s) stars. Revisiting classification criteria and formation scenarios, highlighting i-process nucleosynthesis. | GOSWAMI P.P., RATHOUR R.S. and GOSWAMI A. | ||
2023A&A...674A.130C | 50 | X | 1 | 8 | 1 | Europium enrichment and hierarchical formation of the Galactic halo. | CAVALLO L., CESCUTTI G. and MATTEUCCI F. |
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