TYC 662-217-1 , the SIMBAD biblio

TYC 662-217-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:19:19


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Title First 3 Authors
2016ApJS..224....2H viz 16       D               1 31769 226 The K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8. HUBER D., BRYSON S.T., HAAS M.R., et al.
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.
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.
2018ApJ...863...91F 16       D               1 289 47 New and known moving groups and clusters identified in a Gaia comoving catalog. FAHERTY J.K., BOCHANSKI J.J., GAGNE J., et al.
2019A&A...624A..19B viz 16       D               1 7060 93 The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS. BUDER S., LIND K., NESS M.K., et al.
2020AJ....159..105L viz 16       D               3 158 ~ Discovery of two nearby post-T Tauri stellar associations. LIU J., FANG M. and LIU C.
2020ApJ...903...96G viz 16       D               4 588 27 The µ Tau Association: a 60 Myr old coeval group at 150 pc from the Sun. GAGNE J., DAVID T.J., MAMAJEK E.E., et al.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2022ApJ...928...70C viz 17       D               1 5007 6 Pearls on a String: Numerous Stellar Clusters Strung Along the Same Orbit. CORONADO J., FURNKRANZ V. and RIX H.-W.
2022ApJ...939...94M viz 17       D               1 6091 6 New Coronae and Stellar Associations Revealed by a Clustering Analysis of the Solar Neighborhood. MORANTA L., GAGNE J., COUTURE D., 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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