NGC 2324 147 , the SIMBAD biblio

NGC 2324 147 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST01:50:44


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Title First 3 Authors
1992AJ....104.1892G 185 44 Washington photometry of open cluster giants: nine old disk clusters in the third galactic quadrant. GEISLER D., CLARIA J.J. and MINNITI D.
2001A&A...375...30M viz 85 30 Red giants in open clusters. IX. NGC 2324, 2818, 3960 and 6259. MERMILLIOD J.-C., CLARIA J.J., ANDERSEN J., 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.
2016ApJ...823..114N viz 16       D               1 72935 173 Spectroscopic determination of masses (and implied ages) for red giants. NESS M., HOGG D.W., RIX H.-W., et al.
2016MNRAS.460.3179W viz 16       D               1 77460 19 Distance and extinction determination for APOGEE stars with Bayesian method. WANG J., SHI J., PAN K., et al.
2018AJ....156...18P viz 16       D               1 51824 872 Binary companions of evolved stars in APOGEE DR14: search method and catalog of ∼5000 companions. PRICE-WHELAN A.M., HOGG D.W., RIX H.-W., et al.
2019ApJ...872..137S viz 17       D               1 26099 39 Constraining metallicity-dependent mixing and extra mixing using [C/N] in alpha-rich field giants. SHETRONE M., TAYAR J., JOHNSON J.A., et al.
2019ApJ...879...69T viz 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., 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...900....4S viz 17       D               1 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.
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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