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| BPS CS 30323-0107 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:51:54 |
| 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. | |||||
|
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. | |||
|
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. | ||
|
2011MNRAS.418..284B |
15 | D | 4 | 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 | 15 | D | 1 | 50 | 38 | Lithium abundances in carbon-enhanced metal-poor stars. | MASSERON T., JOHNSON J.A., LUCATELLO S., et al. | ||
| 2012MNRAS.422..849B | 92 | D | F | 2 | 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. | |
|
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. | ||
|
2021ApJ...907...10L |
17 | 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. | ||
|
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. |