NAME Elqui Stream , the SIMBAD biblio

NAME Elqui Stream , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:56:05


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Title First 3 Authors
2018ApJ...862..114S 782       D S   X C       18 50 199 Stellar streams discovered in the Dark Energy Survey. SHIPP N., DRLICA-WAGNER A., BALBINOT E., et al.
2019ApJ...885....3S viz 773     A D S   X C       18 42 49 Proper motions of stellar streams discovered in the Dark Energy Survey. SHIPP N., LI T.S., PACE A.B., et al.
2019MNRAS.490.3508L viz 328           X C F     6 21 68 The Southern Stellar Stream Spectroscopic Survey (S5): Overview, target selection, data reduction, validation, and early science. LI T.S., KOPOSOV S.E., ZUCKER D.B., et al.
2020MNRAS.494..983R 58       D     X         2 224 26 The Milky Way's stellar streams and globular clusters do not align in a Vast Polar Structure. RILEY A.H. and STRIGARI L.E.
2020MNRAS.498.2472K 42           X         1 81 150 Kraken reveals itself - the merger history of the Milky Way reconstructed with the E-MOSAICS simulations. KRUIJSSEN J.M.D., PFEFFER J.L., CHEVANCE M., et al.
2020AJ....160..181J viz 848     A S   X         20 74 47 The Southern Stellar Stream Spectroscopic Survey (S5): chemical Abundances of seven stellar streams. JI A.P., LI T.S., HANSEN T.T., et al.
2021ApJ...909L..26B 269       D     X         7 39 53 Orbital clustering identifies the origins of Galactic stellar streams. BONACA A., NAIDU R.P., CONROY C., et al.
2021ApJ...923..149S 1314       D S   X C       30 17 47 Measuring the mass of the Large Magellanic Cloud With Stellar streams observed by S5. SHIPP N., ERKAL D., DRLICA-WAGNER A., et al.
2022ApJ...926..107M 485       D     X C       11 140 64 The Global Dynamical Atlas of the Milky Way Mergers: Constraints from Gaia EDR3-based Orbits of Globular Clusters, Stellar Streams, and Satellite Galaxies. MALHAN K., IBATA R.A., SHARMA S., et al.
2022ApJ...928...30L 528       D     X         13 53 46 S5: The Orbital and Chemical Properties of One Dozen Stellar Streams. LI T.S., JI A.P., PACE A.B., et al.
2022MNRAS.514.1757P 358       D S   X C       7 30 1 Uniform modelling of the stellar density of thirteen tidal streams within the Galactic halo. PATRICK J.M., KOPOSOV S.E. and WALKER M.G.
2022MNRAS.517.6121V 43           X         1 14 3 The Pristine Inner Galaxy Survey (PIGS) - IV. A photometric metallicity analysis of the Sagittarius dwarf spheroidal galaxy. VITALI S., ARENTSEN A., STARKENBURG E., et al.
2023MNRAS.520.5225M 235       D S   X         5 119 28 galstreams: A library of Milky Way stellar stream footprints and tracks. MATEU C.
2023MNRAS.519.4467J 87               F     2 41 3 Chemical abundances of the Typhon stellar stream. JI A.P., NAIDU R.P., BRAUER K., et al.
2024A&A...687A..46B 108       D         F     1 13 ~ The torsion of stellar streams and the overall shape of galactic gravity's source. BARIEGO-QUINTANA A. and LLANES-ESTRADA F.J.
2024ApJ...974..286A 18       D               1 97 ~ LMC-driven Anisotropic Boosts in Stream-Subhalo Interactions. ARORA A., GARAVITO-CAMARGO N., SANDERSON R.E., et al.
2025MNRAS.537..204P 19       D               1 19 ~ Properties of the lower segment of M31's North West stream. PRESTON J., ERKAL D., COLLINS M.L.M., et al.
2025RNAAS...9...64M 392       D     X         9 175 ~ Origin of the System of Globular Clusters in the Milky Way-Gaia eDR3 Edition. MASSARI D.
2025ApJ...989L..37L 47           X         1 50 ~ Revealing the Origins of Galactic Globular Clusters via their Mg-Al Abundances. LIN S., TANG B., LIU G., et al.
2025A&A...704A.296Y 672       D S   X         14 228 ~ Identifying substructure associations in the Milky Way halo using chemo-kinematic tagging. YOUAKIM K. and LIND K.
2026ApJ...998..114W 300           X         6 32 ~ Detailed Chemical Abundance Analysis of the Brightest Stars in the Turranburra and Willka Yaku Stellar Streams. WEBBER K.B., HANSEN T.T., MARSHALL J.L., et al.
2026A&A...706A.130D viz 600     A D S   X C       11 180 ~ Globular clusters in ORBIT: Complete dynamical characterisation of the Milky Way globular cluster population through updated orbital reconstruction. DE LEO M., ZOCCALI M., OLIVARES-CARVAJAL J., et al.

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