NAME AF06 Stream , the SIMBAD biblio

NAME AF06 Stream , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.7 - 2020.04.05CEST00:02:52


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Title First 3 Authors
2019A&A...631A..47K 1120     A D     X C       24 16 ~ Disentangling the Arcturus stream. KUSHNIRUK I. and BENSBY T.
2018ApJ...863....4L 179           X C       3 22 ~ Tracing the origin of moving groups. I. The γ Leo moving group with high-resolution spectra from the Subaru telescope. LIANG X.L., ZHAO J.K., ZHAO G., et al.
2016MNRAS.460.1356R viz 43           X         1 69 9 Chemical compositions and kinematics of the Hercules stream. RAMYA P., REDDY B.E., LAMBERT D.L., et al.
2015A&A...576A.113Z viz 568     A     X C       13 62 4 Stellar substructures in the solar neighbourhood. IV. Kinematic Group 1 in the Geneva-Copenhagen survey. ZENOVIENE R., TAUTVAISIENE G., NORDSTROEM B., et al.
2014A&A...563A..53Z 477     A S   X C       10 48 4 Stellar substructures in the solar neighbourhood. III. Kinematic group 2 in the Geneva-Copenhagen survey. ZENOVIENE R., TAUTVAISIENE G., NORDSTROEM B., et al.
2014ApJ...787...31Z 478     A     X         12 7 8 Three moving groups detected in the LAMOST DR1 archive. ZHAO J.K., ZHAO G., CHEN Y.Q., et al.
2012MNRAS.425.3188R 1525     A D     X C F     37 55 16 Chemical compositions of stars in two stellar streams from the galactic thick disc. RAMYA P., REDDY B.E. and LAMBERT D.L.
2009ApJ...698..865K viz 78           X         2 250 50 Halo streams in the seventh Sloan Digital Sky Survey data release. KLEMENT R., RIX H.-W., FLYNN C., et al.
2008ApJ...685..261K 78           X       Z 2 20 43 Identifying stellar streams in the first RAVE public data release. KLEMENT R., FUCHS B. and RIX H.-W.
2007A&A...474..857D 115           X         3 14 10 Signatures of star streams in the phase space distribution of nearby halo stars. DETTBARN C., FUCHS B., FLYNN C., et al.
2006A&A...449..533A                   Z 5 77 42 Fine structure in the phase space distribution of nearby subdwarfs. ARIFYANTO M.I. and FUCHS B.

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2020.04.05-00:02:52

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