CVSO 1239 , the SIMBAD biblio

CVSO 1239 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST00:57:35


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Title First 3 Authors
2016AJ....152..198K viz 16       D               1 584 12 The rotation period distributions of 4-10 myr T Tauri stars in Orion OB1: new constraints on pre-main-sequence angular momentum evolution. KARIM M.T., STASSUN K.G., BRICENO C., et al.
2019AJ....157...85B viz 16       D               1 2109 48 The CIDA Variability Survey of Orion OB1 II. Demographics of the young, low-mass stellar populations. BRICENO C., CALVET N., HERNANDEZ 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.
2019A&A...631A.166K viz 16       D               1 1542 3 Discovery of a 21 Myr old stellar population in the Orion complex. KOS J., BLAND-HAWTHORN J., ASPLUND M., et al.
2020AJ....160..268T viz 16       D               1 1158 ~ Statistics of wide pre-main-sequence binaries in the Orion OB1 association. TOKOVININ A., PETR-GOTZENS M.G. and BRICENO C.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2022ApJ...931..156P viz 17       D               1 22106 16 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR 3. II. Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures. PANG X., TANG S.-Y., LI Y., et al.
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.
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.
2023AJ....165..205H viz 17       D               1 847 ~ A LAMOST Spectroscopic Study of T Tauri Stars in the Orion OB1a Subassociation. HERNANDEZ J., ZAMUDIO L.F., BRICENO C., et al.

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