[MIC2016] 46 , the SIMBAD biblio

[MIC2016] 46 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:17:10

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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
2015ApJ...814L...7K 16       D               1 27 36 Triangulum II: possibly a very dense ultra-faint dwarf galaxy. KIRBY E.N., COHEN J.G., SIMON J.D., et al.
2016ApJ...818...40M 16       D               1 62 24 Triangulum II: a very metal-poor and dynamically hot stellar system. MARTIN N.F., IBATA R.A., COLLINS M.L.M., et al.
2017ApJ...838...83K viz 16       D               2 44 87 Triangulum II. Not especially dense after all. KIRBY E.N., COHEN J.G., SIMON J.D., et al.
2017MNRAS.466.3741V 1787     A D S   X C       44 24 15 Gemini/GRACES spectroscopy of stars in Tri II. VENN K.A., STARKENBURG E., MALO L., et al.
2018ApJ...863...89S viz 16       D               1 1159 133 Gaia proper motions and orbits of the ultra-faint Milky Way satellites. SIMON J.D.
2019ApJ...870...83J viz 1520       D S   X C       36 32 61 Chemical abundances in the ultra-faint dwarf galaxies Grus I and Triangulum II: neutron-capture elements as a defining feature of the faintest dwarfs. JI A.P., SIMON J.D., FREBEL A., et al.
2020AJ....160..124M 16       D               2 174 54 Revised and new proper motions for confirmed and candidate Milky Way dwarf galaxies. McCONNACHIE A.W. and VENN K.A.
2021MNRAS.504.1183S 42           X         1 38 4 The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum II, and Coma Berenices UFDs. SITNOVA T.M., MASHONKINA L.I., TATARNIKOV A.M., et al.
2022MNRAS.514.1706B viz 1464       D     X C       34 274 6 Stellar kinematics of dwarf galaxies from multi-epoch spectroscopy: application to Triangulum II. BUTTRY R., PACE A.B., KOPOSOV S.E., et al.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.

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