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| 2MASS J23215820-5211431 , the SIMBAD biblio (13 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST13:01:59 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2006ApJ...652.1585F |
15 | D | 1775 | 155 | Bright metal-poor stars from the Hamburg/ESO survey. I. Selection and follow-up observations from 329 fields. | FREBEL A., CHRISTLIEB N., NORRIS J.E., et al. | |||
| 2016A&A...588A..37H | 488 | D | O X C | 12 | 33 | 24 | Abundances of carbon-enhanced metal-poor stars as constraints on their formation. | HANSEN C.J., NORDSTROM B., HANSEN T.T., 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. | ||
|
2017ApJ...835...81B |
16 | D | 3 | 1801 | 18 | Bright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysis. | BEERS T.C., PLACCO V.M., CAROLLO D., et al. | ||
|
2019A&A...621A.108A |
138 | D | X | 4 | 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. | ||
| 2019ApJ...879...37N | 16 | 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. | ||
| 2020A&A...634A..72S | 16 | D | 5 | 83 | ~ | An empirical metallicity tracer in CEMP and C-normal stars. | SINGH D., HANSEN C.J., BYRGESEN J.S., et al. | ||
|
2020ApJ...894...34D |
16 | 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. | ||
|
2021ApJ...912...52G |
476 | D | X C | 11 | 47 | 15 | R-process-rich stellar streams in the Milky Way. | GULL M., FREBEL A., HINOJOSA K., 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. | ||
| 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. | ||
| 2024MNRAS.530.4712A | 1586 | D | X C F | 34 | 72 | ~ | The oldest stars with low neutron-capture element abundances and origins in ancient dwarf galaxies. | ANDALES H.D., SANTOS FIGUEIREDO A., FIENBERG C.G., et al. |