Cl* Melotte 22 SK 754 , the SIMBAD biblio

Cl* Melotte 22 SK 754 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST21:39:25


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Title First 3 Authors
1991AJ....101..980S 692 64 The search for faint members of the Pleiades. I. A proper motion membership study of the Pleiades to Mv - 12.5. STAUFFER J., KLEMOLA A., PROSSER C., et al.
1991AJ....101.1361P 134 54 The search for faint members of the Pleiades. II. Colors, spectral types, and H-alpha emission line strengths for M dwarfs in the Pleiades, Hyades, and Gliese field. PROSSER C.F., STAUFFER J. and KRAFT R.P.
2007ApJS..172..663S viz 15       D               1 1332 102 Near- and mid-infrared photometry of the Pleiades and a new list of substellar candidate members. STAUFFER J.R., HARTMANN L.W., FAZIO G.G., et al.
2010MNRAS.408..475H viz 15       D               2 1926 134 A large sample of photometric rotation periods for FGK Pleiades stars. HARTMAN J.D., BAKOS G.A., KOVACS G., et al.
2014AJ....148...30K viz 16       D               1 353 20 New BVIC photometry of low-mass Pleiades stars: exploring the effects of rotation on broadband colors. KAMAI B.L., VRBA F.J., STAUFFER J.R., et al.
2016A&A...593L..18C viz 16       D               1 361 1 Pseudomagnitude distances: Application to the Pleiades cluster. CHELLI A. and DUVERT G.
2018MNRAS.476..908F viz 16       D               1 752 35 Stellar activity with LAMOST - II. Chromospheric activity in open clusters. FANG X.-S., ZHAO G., ZHAO J.-K., et al.
2019AJ....157..196K viz 17       D               1 12851 76 Close companions around young stars. KOUNKEL M., COVEY K., MOE M., et al.
2020AJ....160..120J viz 17       D               1 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2020ApJ...903...55P viz 17       D               1 12300 12 Open cluster chemical homogeneity throughout the Milky Way. POOVELIL V.J., ZASOWSKI G., HASSELQUIST S., et al.

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