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| NAME S2 Stream , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:09:42 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2020ApJ...903...25N | 85 | C | 1 | 9 | 35 | Chasing accreted structures within Gaia DR2 using deep learning. | NECIB L., OSTDIEK B., LISANTI M., et al. | ||
|
2021MNRAS.500..889A |
4932 | T A | D | S X C | 116 | 83 | 32 |
The S2 stream: the shreds of a primitive dwarf galaxy. |
AGUADO D.S., MYEONG G.C., BELOKUROV V., et al. |
| 2021ApJ...908L...8A | 86 | C | 1 | 24 | 49 | Elevated r-process enrichment in Gaia Sausage and Sequoia. | AGUADO D.S., BELOKUROV V., MYEONG G.C., et al. | ||
| 2021MNRAS.505..200M | 42 | X | 1 | 16 | 7 | The evolution of Lithium: implications of a universal Spite plateau. | MATTEUCCI F., MOLERO M., AGUADO D.S., et al. | ||
|
2021MNRAS.507...43S |
42 | X | 1 | 257 | 14 | The GALAH survey: accreted stars also inhabit the Spite plateau. | SIMPSON J.D., MARTELL S.L., BUDER S., et al. | ||
| 2022A&A...659A..61D | 43 | X | 1 | 10 | 8 | Substructures, resonances, and debris streams. A new constraint on the inner shape of the Galactic dark halo. | DODD E., HELMI A. and KOPPELMAN H.H. | ||
| 2022ApJ...938...21M | 47 | X | 1 | 7 | 31 | Milky Way's Eccentric Constituents with Gaia, APOGEE, and GALAH. | MYEONG G.C., BELOKUROV V., AGUADO D.S., et al. | ||
| 2024MNRAS.529.2413U | 45 | X | 1 | 26 | ~ | Multiple populations and a CH star found in the 300S globular cluster stellar stream. | USMAN S.A., JI A.P., LI T.S., et al. | ||
| 2024A&A...690A.245B | 45 | X | 1 | 7 | ~ | A coherent view of Li depletion and angular momentum transport to explain the Li plateau - from Population II to Population I stars. | BORISOV S., CHARBONNEL C., PRANTZOS N., et al. | ||
| 2024A&A...691A.277W | 161 | A | X | 4 | 11 | ~ | First measurement of the triaxiality of the inner dark matter halo of the Milky Way. | WOUDENBERG H.C. and HELMI A. |