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Published June 1, 2020 | Version v1
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Relative Importance of Convective Uncertainties in Massive Stars

  • 1. Keele University, Keele, Staffordshire ST5 5BG, UK
  • 2. Steward Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson AZ 85721, USA
  • 3. Department of Astronomy, University of Geneva, Ch. Maillettes 51, 1290 Versoix, Switzerland

Description

Inlist used for the paper: "Relative Importance of Convective Uncertainties in Massive Stars" (arXiv:2006.01877)

The stellar tracks and profile outputs are available on http://www.astro.keele.ac.uk/shyne/datasets/convective-boundary-mixing-uncertainties

This work was done with MESA version 10398.

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