HD 61288 , the SIMBAD biblio

HD 61288 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:00:42


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Title First 3 Authors
1967MNSSA..26...30W 212 20 Photometric photometry of NGC 2451. WILLIAMS P.M.
1976ApJ...205..807H 264 65 The frequency of peculiar A and metallic-line stars in open clusters. HARTOOG M.R.
1982MSS...C03....0H viz 14       D               1 30313 ~ Catalogue of two-dimensional spectral types for the HD stars, Vol. 3 HOUK N.
1998A&A...340..402B 142 28 The nature of some doubtful open clusters as revealed by Hipparcos. BAUMGARDT H.
2012AstL...38..694G viz 15       D               1 20524 9 Spatial distribution and kinematics of OB stars. GONTCHAROV G.A.
1993yCat.3135....0C viz 14       D               1 252979 52 VizieR Online Data Catalog: Henry Draper Catalogue and Extension, published in Ann. Harvard Obs. 91-100 (1918-1925) CANNON A.J. and PICKERING E.C.
2014ASPC..485..223B viz 15       D               1 465820 45 The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements BOURGES L., LAFRASSE S., MELLA G., et al.
2018A&A...615A..49C viz 16       D               1 224763 54 Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al.
2018A&A...620A.172Z viz 16       D               1 127610 99 3D mapping of young stars in the solar neighbourhood with Gaia DR2. ZARI E., HASHEMI H., BROWN A.G.A., et al.
2019MNRAS.490.3158C viz 16       D               1 465839 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., 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.
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.

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