NAME gam Leo Moving Group , the SIMBAD biblio

NAME gam Leo Moving Group , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST16:55:56


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Title First 3 Authors
2018ApJ...863....4L 827 T   A     X C       19 22 2 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.
2018ApJ...868..105Z 40           X         1 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.
2019A&A...631A..47K 707       D     X         18 16 ~ Disentangling the Arcturus stream. KUSHNIRUK I. and BENSBY T.
2020ApJ...890...85L 58       D     X         2 10 6 Dissecting the phase space snail shell. LI Z.-Y. and SHEN J.
2020AJ....159..196L 41           X         1 21 ~ A new moving group in the Local Arm. LIANG X., ZHAO J., CHEN Y., et al.
2021MNRAS.505.2561C 59       D     X         2 16 ~ Dynamically produced moving groups in interacting simulations. CRAIG P., CHAKRABARTI S., NEWBERG H., et al.
2021ApJ...922..105Y 42           X         1 10 8 Tracing the origin of moving groups. III. Detecting moving groups in LAMOST DR7. YANG Y., ZHAO J., ZHANG J., et al.
2022MNRAS.512.6201M 85               F     2 9 4 The velocity distribution of white dwarfs in Gaia EDR3. MIKKOLA D., McMILLAN P.J., HOBBS D., et al.
2023MNRAS.521..208M 192       D     X   F     4 12 1 Chemodynamical ages of small-scale kinematic structures of the galactic disc in the solar neighbourhood from ∼250 000 K and M dwarfs. MEDAN I. and LEPINE S.
2024AJ....168..277L 376       D     X         9 13 ~ Moving Groups in the Solar Neighborhood with Gaia, APOGEE, GALAH, and LAMOST: Dynamical Effects Gather Gas and the Ensuing Star Formation Plays an Important Role in Shaping the Stellar Velocity Distributions. LIANG X., YOON S.-J. and ZHAO J.
2025ApJS..281...36W 112       D     X         3 22 ~ Planets Across Space and Time (PAST). VIII. Kinematic Characterization and Identification of Radial Velocity Variables for the LAMOST-Gaia-TESS Stars. WU D., CHEN D.-C., XIE J.-W., et al.

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