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

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We 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.
Original languageEnglish
JournalRediscovering our Galaxy, Proceedings of the International Astronomical Union, IAU Symposium
Volume334
Pages (from-to)178-181
DOIs
Publication statusPublished - 1 Aug 2018
Externally publishedYes

    Research areas

  • Stars: interiors, stars: evolution, methods: numerical

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