HD 25402B , the SIMBAD biblio

HD 25402B , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:30:10


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Title First 3 Authors
2011MNRAS.411..117K 39           X         1 28 59 A search for new members of the β Pictoris, Tucana–Horologium and ε Cha moving groups in the RAVE data base. KISS L.L., MOOR A., SZALAI T., et al.
2020AJ....159..166U viz 16       D               1 615 26 Analysis of membership probability in nearby young moving groups with Gaia DR2. UJJWAL K., KARTHA S.S., MATHEW B., et al.
2020MNRAS.496.5176D 16       D               2 304 38 Wide binaries are rare in open clusters. DEACON N.R. and KRAUS A.L.
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2022MNRAS.511.6179L viz 17       D               1 2244 3 Low-mass members of nearby young stellar moving groups from Gaia EDR3. LEE J., SONG I. and MURPHY S.J.
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...663A.144B viz 43           X         1 127 15 New binaries from the SHINE survey. BONAVITA M., GRATTON R., DESIDERA S., et al.
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.
2023ApJ...945..114P viz 17       D               2 391 1 Examining the Rotation Period Distribution of the 40 Myr Tucana-Horologium Association with TESS. POPINCHALK M., FAHERTY J.K., CURTIS J.L., et al.
2023AJ....165..267H viz 17       D               1 64663 1 Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., 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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