The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations
Author:
Funder
NSF
NASA
European Union Horizon 2020
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/874/i=2/a=180/pdf
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3. 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
4. A compilation of charged-particle induced thermonuclear reaction rates
5. Faint stellar photometry in clusters. II - NGC 6791 and NGC 6535
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