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MESA model files and scripts for: 'An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models'

  • Ebraheem Farag (Contributor)
  • Christopher J. Fontes (Contributor)
  • Francis Timmes (Contributor)
  • Earl P. Bellinger (Contributor)
  • Joyce A. Guzik (Contributor)
  • Evan B. Bauer (Contributor)
  • Suzannah R. Wood (Contributor)
  • Katie Mussack (Contributor)
  • Peter Hakel (Contributor)
  • James Colgan (Contributor)
  • David P. Kilcrease (Contributor)
  • Manolo E. Sherrill (Contributor)
  • Tryston C. Raecke (Contributor)
  • Morgan T. Chidester (Contributor)

Dataset

Description

MESA model files and plotting scripts for plots seen in 'An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models'. https://iopscience.iop.org/article/10.3847/1538-4357/ad4355 Models were run using MESA version r22.11.1, with fixes to the bugs documented at https://docs.mesastar.org/en/release-r24.03.1/known_bugs.html#r22-11-1. We use mesasdk-x86_64-linux-22.6.1.tar.gz sdk available at http://user.astro.wisc.edu/~townsend/resource/download/mesasdk We do not include the opacity tables here but they will be available in the next MESA release version and at http://aphysics2.lanl.gov/opacity/lanl. *(In future solar modeling work, we recommend users use 'rmid' (cell centered radius in Rsun) instead of 'radius' (cell edge/face radius in Rsun) as all structural variables are typically defined at the cell center. Look into $MESA_DIR/star/defaults/profile_columns.list and ensure you are always consistently using cell centered or cell-faced variables with each other.)*
Date made availableMar 8 2024
PublisherZenodo

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