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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S334(13), p. 178-181

DOI: 10.1017/s1743921317008894

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Using low-mass stars as a tool: efforts towards precise models

Journal article published in 2017 by Achim Weiss ORCID, Victor Silva Aguirre, Jørgen Christensen-Dalsgaard ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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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.

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