Cl* Melotte 22 AK V-252 , the SIMBAD biblio

Cl* Melotte 22 AK V-252 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST08:52:20


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Title First 3 Authors
1997A&A...320...74M viz 116 11 Investigation of the Pleiades cluster. III. Additional corona members. MERMILLIOD J.-C., BRATSCHI P. and MAYOR M.
2009A&A...498..949M viz 15       D               1 1252 96 Catalogues of radial and rotational velocities of 1253 F-K dwarfs in 13 nearby open clusters. MERMILLIOD J.-C., MAYOR M. and UDRY S.
2017AJ....153..257O viz 16       D               1 10625 142 Comoving stars in Gaia DR1: an abundance of very wide separation comoving pairs. OH S., PRICE-WHELAN A.M., HOGG D.W., et al.
2017A&A...601A..19G viz 16       D               1 1218 88 Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects. GAIA COLLABORATION, VAN LEEUWEN F., VALLENARI A., et al.
2018ApJ...856...23G viz 16       D               1 1600 367 BANYAN. XI. The BANYAN Σ multivariate Bayesian algorithm to identify members of young associations with 150 pc. GAGNE J., MAMAJEK E.E., MALO L., et al.
2018AJ....155..149B viz 16       D               1 9764 5 Fundamental properties of co-moving stars observed by Gaia. BOCHANSKI J.J., FAHERTY J.K., GAGNE J., et al.
2019PASP..131d4101G viz 16       D               1 1456 10 An investigation of the Pleiades cluster Using machine learning. GAO X.-H.
2019AJ....158..122K viz 16       D               1 290057 150 Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. KOUNKEL M. and COVEY K.
2021ApJS..257...46G viz 17       D               1 10775 37 Stellar rotation in the Gaia era: revised open clusters' sequences. GODOY-RIVERA D., PINSONNEAULT M.H. and REBULL L.M.
2022ApJS..262....7H viz 17       D               1 134735 19 A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun. HE Z., WANG K., LUO Y., et al.
2024AJ....167..210V viz 18       D               1 7289 ~ The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. VACH S., ZHOU G., HUANG C.X., et al.

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