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| SMSS J195931.70-643529.3 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST16:47:10 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2015ApJ...807..171J |
16 | D | 1 | 131 | 106 | High-resolution spectroscopic study of extremely metal-poor star candidates from the SkyMapper survey. | JACOBSON H.R., KELLER S., FREBEL A., et al. | ||
|
2018AJ....156..179R |
16 | D | 1 | 90 | 63 | Kinematics of highly r-process-enhanced field stars: evidence for an accretion origin and detection of several groups from disrupted satellites. | ROEDERER I.U., HATTORI K. and VALLURI M. | ||
|
2019ApJ...870..122P |
16 | D | 1 | 859 | 1 | The r-process Alliance: spectroscopic follow-up of low-metallicity star candidates from the Best & Brightest Survey. | PLACCO V.M., SANTUCCI R.M., BEERS T.C., et al. | ||
|
2019ApJ...882...40J |
16 | D | 2 | 210 | 41 | The lanthanide fraction distribution in metal-poor stars: a test of neutron star mergers as the dominant r-process site. | JI A.P., DROUT M.R. and HANSEN T.T. | ||
|
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. | ||
|
2021MNRAS.503.2539C |
17 | D | 1 | 478 | 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. | ||
|
2022ApJ...926...26S |
17 | D | 1 | 6507 | 18 | Dynamically Tagged Groups of Metal-poor Stars from the Best and Brightest Survey. | SHANK D., BEERS T.C., PLACCO V.M., et al. | ||
|
2023ApJ...943...23S |
17 | D | 1 | 1792 | 5 | The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars. | SHANK D., BEERS T.C., PLACCO V.M., et al. | ||
|
2023ApJ...946...48H |
17 | D | 2 | 181 | 5 | Finding r-II Sibling Stars in the Milky Way with the Greedy Optimistic Clustering Algorithm. | HATTORI K., OKUNO A. and ROEDERER I.U. |