NAME Hrid Stream , the SIMBAD biblio

NAME Hrid Stream , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:36:28


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Title First 3 Authors
2021ApJ...914..123I viz 359     A S   X C       7 6030 82 Charting the Galactic acceleration field. I. A search for stellar streams with Gaia DR2 and EDR3 with follow-up from ESPaDOnS and UVES. IBATA R., MALHAN K., MARTIN N., et al.
2022MNRAS.510.1945M 43           X         1 7 1 L-GALAXIES 2020: the formation and chemical evolution of stellar haloes in Milky Way analogues and galaxy clusters. MURPHY G.G., YATES R.M. and MOHAMED S.S.
2022MNRAS.511.1714T 230       D     X C       5 24 5 The high-velocity clouds above the disc of the outer Milky Way: misty precipitating gas in a region roiled by stellar streams. TRIPP T.M.
2022ApJ...926..107M 17       D               3 140 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.
2023A&A...669A.136G 87           X         2 82 1 Gaia-IGRINS synergy: Orbits of newly identified Milky Way star clusters. GARRO E.R., FERNANDEZ-TRINCADO J.G., MINNITI D., et al.
2023MNRAS.520.5225M 104       D S             3 119 28 galstreams: A library of Milky Way stellar stream footprints and tracks. MATEU C.
2023ApJ...954..215Y 17       D               1 17 ~ Stream Fanning and Bifurcations: Observable Signatures of Resonances in Stellar Stream Morphology. YAVETZ T.D., JOHNSTON K.V., PEARSON S., et al.
2024MNRAS.529.4745S 108       D     X         3 28 ~ VIA MACHINAE 2.0: Full-sky, model-agnostic search for stellar streams in Gaia DR2. SHIH D., BUCKLEY M.R. and NECIB L.
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.
2025A&A...704A.296Y 485       D S   X         10 228 ~ Identifying substructure associations in the Milky Way halo using chemo-kinematic tagging. YOUAKIM K. and LIND K.

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