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| UCAC4 728-064676 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST11:56:55 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2018AJ....156..179R 
|
40 | X | 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. | ||
| 2018ApJ...866..121H | 16 | D | 1 | 39 | 25 | Old, metal-poor extreme velocity stars in the solar neighborhood. | HATTORI K., VALLURI M., BELL E.F., et al. | ||
| 2018MNRAS.481.1028H | 178 | D | C F | 4 | 14 | 16 | The fastest travel together: chemical tagging of the fastest stars in Gaia DR2 to the stellar halo. | HAWKINS K. and WYSE R.F.G. | |
| 2020RAA....20...42L | 16 | D | 1 | 49 | ~ | Three New Late-type Hypervelocity Star Candidates from Gaia DR2 with Refined Selection Criteria. | LI J., JIA S., GAO Y., et al. | ||
|
2022AJ....163..252R
|
17 | D | 3 | 22 | 5 | The Chemical Composition of Extreme-velocity Stars. | REGGIANI H., JI A.P., SCHLAUFMAN K.C., 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. | ||
|
2024MNRAS.532.2875N
|
18 | D | 1 | 48 | ~ | A detailed chemical study of the extreme velocity stars in the galaxy. | NELSON T., HAWKINS K., REGGIANI H., 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. |
