UCAC2 21339622 , the SIMBAD biblio

UCAC2 21339622 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:39:53


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Title First 3 Authors
2016MNRAS.461..794P viz 16       D               1 802 260 The star formation history and accretion-disc fraction among the K-type members of the Scorpius-Centaurus OB association. PECAUT M.J. and MAMAJEK E.E.
2018MNRAS.473.1231A 96       D         F     2 138 7 Identification of young stellar variables with KELT for K2 - II. The Upper Scorpius association. ANSDELL M., OELKERS R.J., RODRIGUEZ J.E., et al.
2018MNRAS.477L..50G viz 16       D               1 1321 7 Three-dimensional structure of the Upper Scorpius association with the Gaia first data release. GALLI P.A.B., JONCOUR I. and MORAUX E.
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.
2020AJ....160...44L viz 16       D               1 2652 55 Refining the census of the Upper Scorpius association with Gaia. LUHMAN K.L. and ESPLIN T.L.
2022A&A...657A..53B viz 17       D               2 376 1 Unveiling wide-orbit companions to K-type stars in Sco-Cen with Gaia EDR3. BOHN A.J., GINSKI C., KENWORTHY M.A., 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.
2022A&A...667A.163M viz 17       D               1 2829 10 The star formation history of Upper Scorpius and Ophiuchus A 7D picture: positions, kinematics, and dynamical traceback ages. MIRET-ROIG N., GALLI P.A.B., OLIVARES J., 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...677A..59R viz 17       D               1 13197 ~ Significance mode analysis (SigMA) for hierarchical structures An application to the Sco-Cen OB association. RATZENBOCK S., GROSSSCHEDL J.E., MOLLER T., et al.

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