NAME Kapteyn Moving Group , the SIMBAD biblio

NAME Kapteyn Moving Group , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST22:19:03


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Title First 3 Authors
1996AJ....112.1595E 233 101 Star streams and galactic structure. EGGEN O.J.
2010AJ....139..636W 1830 T   A     X C       47 25 39 Evidence of tidal debris from ω Cen in the Kapteyn group. WYLIE-DE BOER E., FREEMAN K. and WILLIAMS M.
2015ApJ...808..103N viz 2948     A     X C       75 56 14 The
Kapteyn moving group is not tidal debris from ω Centauri.
NAVARRETE C., CHANAME J., RAMIREZ I., et al.
2015MNRAS.451..705M 609     A     X C F     14 4 10 Resonant trapping in the galactic disc and halo and its relation with moving groups. MORENO E., PICHARDO B. and SCHUSTER W.J.
2015AJ....150..128R 39           X         1 7 7 New signatures of the Milky Way formation in the local halo and inner-halo streamers in the era of Gaia. RE FIORENTIN P., LATTANZI M.G., SPAGNA A., et al.
2016ApJ...821...81G 79           X         2 23 32 Living with a red dwarf: rotation and X-ray and ultraviolet properties of the halo population Kapteyn's star. GUINAN E.F., ENGLE S.G. and DURBIN A.
2018MNRAS.478.5449M 88           X         2 10 81 Discovery of new retrograde substructures: the shards of ω Centauri? MYEONG G.C., EVANS N.W., BELOKUROV V., et al.
2018ApJ...865..129R viz 41           X         1 25 41 The r-process Alliance: a comprehensive abundance analysis of HD 222925, a metal-poor star with an extreme r-process enhancement of [Eu/H] = -0.14. ROEDERER I.U., SAKARI C.M., PLACCO V.M., et al.
2018ApJ...868..105Z 161           X         4 28 2 Tracing the origin of moving groups. II. Chemical abundance of six stars in the halo stream LAMOST-N1. ZHAO J.K., ZHAO G., AOKI W., et al.
2019MNRAS.488.1235M 47           X         1 49 307 Evidence for two early accretion events that built the Milky Way stellar halo. MYEONG G.C., VASILIEV E., IORIO G., et al.
2019PASP..131k4201C 422       D     X C       10 319 ~ A GALEX far-ultraviolet study of dwarf stars in moving groups. COCHRANE K.M. and SMITH G.H.
2021AJ....162..109S viz 84           X         2 60 ~ Combining astrometry and elemental abundances: the case of the candidate pre-Gaia halo moving groups G03-37, G18-39, and G21-22. SCHULER S.C., ANDREWS J.J., CLANZY V.R., et al.

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