Chemical abundance analysis of the open clusters Berkeley 32, NGC 752, Hyades, and Praesepe
A&A, 535 (2011) A30
Published online: 2011-10-27
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LIMITATIONS OF CN AND CH MOLECULAR BAND STRENGTHS AT HIGH METALLICITIES: A CASE STUDY IN NGC 6791
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THE DISTANCES TO OPEN CLUSTERS FROM MAIN-SEQUENCE FITTING. V. EXTENSION OF COLOR CALIBRATION AND TEST USING COOL AND METAL-RICH STARS IN NGC 6791
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The old, metal-poor, anticentre open cluster Trumpler 5★
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INITIAL–FINAL MASS RELATION FOR 3 TO 4M⊙PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099
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CHEMICAL ABUNDANCES OF MEMBER STARS IN THE OPEN CLUSTER NGC 2632 (PRAESEPE)
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CHARACTERIZATION OF THE PRAESEPE STAR CLUSTER BY PHOTOMETRY AND PROPER MOTIONS WITH 2MASS, PPMXL, AND Pan-STARRS
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On the metallicity of open clusters
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Abundance analysis of red clump stars in the old, inner disc, open cluster NGC 4337: a twin of NGC 752?
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