NGC 2682 49 , the SIMBAD biblio

NGC 2682 49 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:46:54


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Title First 3 Authors
1977A&AS...27...89S 14       D               1 1852 182 Membership of the open cluster M 67. SANDERS W.L.
1986AJ.....92.1100M 209 129 Precise radial velocities of late-type stars in the open clusters M 11 and M 67. MATHIEU R.D., LATHAM D.W., GRIFFIN R.F., et al.
1989AJ.....98..227G 654 176 Relative proper motions and the stellar velocity dispersion of the open cluster M 67. GIRARD T.M., GRUNDY W.M., LOPEZ C.E., et al.
1993A&AS..100..243Z viz 680 29 Study of proper motions in the region of the open cluster M67 and membership of stars. ZHAO J.L., TIAN K.P., PAN R.-S., et al.
1993AJ....106..181M viz 14       D               1 1441 326 CCD photometry of old open cluster M 67. MONTGOMERY K.A., MARSCHALL L.A. and JANES K.A.
1996AJ....112..628F viz 6562 218 Deep wide-field spectrophotometry of the open cluster M67. FAN X., BURSTEIN D., CHEN J.-S., et al.
1998BaltA...7..369B viz 280 11 CCD photometry of the M67 cluster in the Vilnius photometric system. BOYLE R.P., KAZLAUSKAS A., VANSEVICIUS V., et al.
2004AJ....127.1513S viz 111 52 The integrated spectrum of M67 and the spectroscopic age of M32. SCHIAVON R.P., CALDWELL N. and ROSE J.A.
1940ApJ....91..244E 153 17 Proper motions in the galactic cluster M 67. EBBIGHAUSEN E.G.
2010A&A...516A...3K viz 15       D               1 26582 13 Kinematic parameters and membership probabilities of open clusters in the Bordeaux PM2000 catalogue. KRONE-MARTINS A., SOUBIRAN C., DUCOURANT C., et al.
2015A&A...580A..23P viz 16       D               2 60854 134 A new catalogue of Stroemgren-Crawford uvbyβ photometry. PAUNZEN E.
2015AJ....150...97G viz 16       D               1 1279 98 Stellar radial velocities in the old open cluster M67 (NGC 2682). I. Memberships, binaries, and kinematics. GELLER A.M., LATHAM D.W. and MATHIEU R.D.
2016ApJS..224....2H viz 16       D               1 31769 226 The K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8. HUBER D., BRYSON S.T., HAAS M.R., et al.
2016MNRAS.459.1060G viz 16       D               1 674 7 Variability among stars in the M 67 field from Kepler/K2-Campaign-5 light curves. GONZALEZ G.
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.
2018AJ....156..142D viz 16       D               1 1381 47 The Open Cluster Chemical Abundances and Mapping survey. II. Precision cluster abundances for APOGEE using SDSS DR14. DONOR J., FRINCHABOY P.M., CUNHA K., et al.
2019ApJ...879...69T viz 16       D               1 222610 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., 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.
2020ApJ...903...55P viz 16       D               1 12301 12 Open cluster chemical homogeneity throughout the Milky Way. POOVELIL V.J., ZASOWSKI G., HASSELQUIST S., et al.
2020ApJS..251...15Z viz 16       D               1 20886 38 Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution Spectroscopic observations. ZONG W., FU J.-N., DE CAT P., et al.
2021RAA....21..292W viz 17       D               4 9395 19 LAMOST Time-Domain survey: first results of four K2 plates. WANG S., ZHANG H.-T., BAI Z.-R., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2023ApJS..264...12H viz 17       D               2 1697 2 Stellar Chromospheric Activities Revealed from the LAMOST-K2 Time-domain Survey. HAN H., WANG S., BAI Y., et al.

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