The Influence of the Metal Mass Fraction Z, Age, and Mixing-length Parameter on the RGB Bump Magnitude for the M4 Cluster
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/869/i=2/a=109/pdf
Reference47 articles.
1. The Main Sequence of the Globular Cluster M4=NGC 6121 From CCD NTT Photometry
2. Theoretical Uncertainties in Red Giant Branch Evolution: The Red Giant Branch Bump
3. ON THE DISTANCE OF THE GLOBULAR CLUSTER M4 (NGC 6121) USING RR LYRAE STARS. I. OPTICAL AND NEAR-INFRARED PERIOD-LUMINOSITY AND PERIOD-WESENHEIT RELATIONS
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