CPD-24 2200 , the SIMBAD biblio

CPD-24 2200 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:14:32


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Title First 3 Authors
1950ApJ...112..240J 73 22 The color-magnitude array for the galactic cluster NGC 2362. JOHNSON H.L.
1996MNRAS.281.1341B 77 27 CCD Stromgren photometry of NGC 2362. BALONA L.A. and LANEY C.D.
2006ApJ...646..269D viz 15       D               1 175 14 Multiwavelength analysis of the young open cluster NGC 2362. DELGADO A.J., GONZALEZ-MARTIN O., ALFARO E.J., et al.
2007AJ....133.2072D viz 15       D               345 75 Spitzer observations of NGC 2362: primordial disks at 5 Myr. DAHM S.E. and HILLENBRAND L.A.
2009ApJ...698....1C viz 15       D               1 358 132 The last gasp of gas giant planet formation: a Spitzer study of the 5 Myr old cluster NGC 2362. CURRIE T., LADA C.J., PLAVCHAN P., et al.
2011A&A...531A.141D viz 15       D               2 666 16 Physical parameters of pre-main sequence stars in open clusters. DELGADO A.J., ALFARO E.J. and YUN J.L.
2013MNRAS.434..806B viz 15       D               1 4741 204 Pre-main-sequence isochrones - II. Revising star and planet formation time-scales. BELL C.P.M., NAYLOR T., MAYNE N.J., et al.
2013ApJS..209...32B viz 15       D               1 8196 71 Identifying young stars in massive star-forming regions for the MYStIX project. BROOS P.S., GETMAN K.V., POVICH M.S., et al.
2018A&A...618A..93C viz 16       D               1 87620 517 A Gaia DR2 view of the open cluster population in the Milky Way. CANTAT-GAUDIN T., JORDI C., VALLENARI A., et al.
2020A&A...633A..99C viz 16       D               1 257585 169 Clusters and mirages: cataloguing stellar aggregates in the Milky Way. CANTAT-GAUDIN T. and ANDERS F.
2020A&A...640A...1C viz 16       D               1 235399 241 Painting a portrait of the Galactic disc with its stellar clusters. CANTAT-GAUDIN T., ANDERS F., CASTRO-GINARD A., et al.
2021ApJ...916...32G viz 17       D               1 1084 20 X-ray superflares from pre-main-sequence stars: flare energetics and frequency. GETMAN K.V. and FEIGELSON E.D.

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