Published November 2, 2023 | Version v1
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Inlist and Source Code Files for "Fossil Signatures of Main-sequence Convective Core Overshoot Estimated through Asteroseismic Analyses"

  • 1. ROR icon Yale University
  • 2. ROR icon University of Hawaii System

Description

MESA (r12778) and GYRE (version 6.0) inlist files used in the work described in "Fossil Signatures of Main-sequence Convective Core Overshoot Estimated through Asteroseismic Analyses".

Two subdirectories are provided in the archive:

1) The directory called "inlists" contains different MESA inlist files for different evolutionary period (pms=pre main sequence, ms=main sequence, and rgb=red giant branch) of the stellar model. The file named "inlist_0all" is applied to all evolutionary periods. The different inlist files for the different evolutionary states are called by putting their names in the "inlist" file, for example the include file named "inlist" evolves a MESA model from the pre main sequence until ZAMS (using the stop_near_zams = .true. option in the "inlist_1pms" file). An example gyre (version 6.0) inlist is also included in the "inlists" subdirectory.  The Python scripts used to evaluate the matrix elements (which are used to determine the dipolar mixed-mode frequencies) discussed in this work are available at https://gitlab.com/darthoctopus/mesatricks. 

2) Custom stopping conditions (used for stopping a model before the red giant branch) as well as a custom diffusion cutoff (see Viani et al. 2018, ApJ, 858, 28) are included in the run_star_extras.f file in the "src" subdirectory. 

Files

Zenodo_Fossil_Signatures_of_Overshoot.zip

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