Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S334(13), p. 178-181
DOI: 10.1017/s1743921317008894
Full text: Unavailable
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.