TYC 3338-277-1 , the SIMBAD biblio

TYC 3338-277-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:44:37


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Title First 3 Authors
2000MNRAS.313...43H viz 14       D               1 3287 16 OB association members in the ACT and TRC catalogues. HOOGERWERF R.
2010ApJS..187..447C 40           X         1 4 18 Chandra observations of comets 8p/Tuttle and 17p/Holmes during solar minimum. CHRISTIAN D.J., BODEWITS D., LISSE C.M., 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.
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.
2021A&A...645A..84M viz 17       D               1 7942 60 Extended stellar systems in the solar neighborhood. V. Discovery of coronae of nearby star clusters. MEINGAST S., ALVES J. and ROTTENSTEINER A.
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.
2023ApJS..265...12Q viz 17       D               1 58898 5 Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc. QIN S., ZHONG J., TANG T., et al.
2023A&A...678A..75Z viz 17       D               1 27445 ~ Young nearby open clusters and their luminosity functions. ZERJAL M., LODIEU N., PEREZ-GARRIDO A., 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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