volume 13, issue S334, P178-181 2017
DOI: 10.1017/s1743921317008894
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Achim Weiss, Victor Silva Aguirre, Jørgen Christensen-Dalsgaard

Abstract: AbstractWe present results of an on-going effort to identify the minimum level of systematic, purely numerical differences in low-mass stellar models on the Red Giant Branch, by comparing models in selected phases for pre-defined physical input assumptions.