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[AAS2009] S 11-13 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST00:38:53 |
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 |
---|---|---|---|---|---|---|---|---|---|
2009AJ....137.3100W | 15 | D | 1 | 7115 | 223 | Stellar velocities in the Carina, Fornax, Sculptor, and Sextans dSph galaxies: data from the Magellan/MMFS survey. | WALKER M.G., MATEO M. and OLSZEWSKI E.W. | ||
2009A&A...502..569A | 16 | D | 6 | 23 | 88 | Chemical composition of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy. | AOKI W., ARIMOTO N., SADAKANE K., et al. | ||
2010A&A...524A..58T | 16 | D | 1 | 45 | 138 | Extremely metal-poor stars in classical dwarf spheroidal galaxies: Fornax, Sculptor, and Sextans. | TAFELMEYER M., JABLONKA P., HILL V., et al. | ||
2011MNRAS.411.1013B | 15 | D | 1 | 187 | 143 | Study of the Sextans dwarf spheroidal galaxy from the DART Ca II triplet survey. | BATTAGLIA G., TOLSTOY E., HELMI A., et al. | ||
2012ApJ...759..111K | 193 | X C | 4 | 28 | 24 | The chemical signature of a relic star cluster in the Sextans dwarf spheroidal galaxy–Implications for near-field cosmology. | KARLSSON T., BLAND-HAWTHORN J., FREEMAN K.C., et al. | ||
2018A&A...609A..53C | 16 | D | 1 | 1597 | 15 | Tracing the stellar component of low surface brightness Milky Way dwarf galaxies to their outskirts. I. Sextans. | CICUENDEZ L., BATTAGLIA G., IRWIN M., et al. | ||
2020A&A...636A.111A | 826 | D | X | 20 | 44 | ~ | Chemical abundance analysis of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy. | AOKI M., AOKI W. and FRANCOIS P. | |
2020A&A...644A..75L | 102 | D | X | 3 | 18 | ~ | Homogeneity in the early chemical evolution of the Sextans dwarf spheroidal galaxy. | LUCCHESI R., LARDO C., PRIMAS F., et al. | |
2022MNRAS.509.3626M | 18 | D | 4 | 18 | 7 | The formation of the Milky Way halo and its dwarf satellites: A NLTE-1D abundance analysis. V. The Sextans galaxy. | MASHONKINA L., PAKHOMOV Y.V., SITNOVA T., et al. |