CPD-53 6255 , the SIMBAD biblio

CPD-53 6255 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST15:15:24


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Title First 3 Authors
1978AJ.....83.1424D 40 33 DDO photometry of giants in four southern open clusters. DAWSON D.W.
1979A&A....79...11M 15 ~ Red giants in open clusters. II. Orbits of the spectroscopic binaries in NGC 2360, 2437, 2447, 5822, 5823, and 6475. MERMILLIOD J.-C., MAYOR M., ANDERSEN J., et al.
1985MNRAS.214..229C 15 19 New photometric data for the red giants in the open cluster NGC 5822: membership, chemical composition and physical properties. CLARIA J.J. and LAPASSET E.
1990A&A...237...61M 91 75 Red giants in open clusters. III. Binarity and stelllar evolution in five intermediate-age clusters: NGC 2360, 2423, 5822, 6811 and IC 4756. MERMILLIOD J.-C. and MAYOR M.
1993PASP..105...78T viz 14       D               1 617 34 A photometric analysis of the intermediate-age open cluster NGC 5822. TWAROG B.A., ANTHONY-TWAROG B.J. and McCLURE R.D.
1995A&A...296..709V 1 39 202 Tidal circularization and the eccentricity of binaries containing giant stars. VERBUNT F. and PHINNEY E.S.
2004A&A...424..727P viz 15       D               1 3570 525 SB9: The ninth catalogue of spectroscopic binary orbits. POURBAIX D., TOKOVININ A.A., BATTEN A.H., et al.
2008A&A...485..303M viz 15       D               1474 156 Red giants in open clusters. XIV. Mean radial velocities for 1309 stars and 166 open clusters. MERMILLIOD J.C., MAYOR M. and UDRY S.
2008AJ....136..118F viz 15       D               1 3514 68 Open clusters as galactic disk tracers. I. Project motivation, cluster membership, and bulk three-dimensional kinematics. FRINCHABOY P.M. and MAJEWSKI S.R.
2014AJ....148...83S viz 803   K   D     X C       20 72 5 High-resolution spectroscopic observations of binary stars and yellow stragglers in three open clusters : NGC 2360, NGC 3680, and NGC 5822. SALES SILVA J.V., PENA SUAREZ V.J., KATIME SANTRICH O.J., et al.
2018A&A...615A..49C viz 16       D               1 224764 54 Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al.

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