Published July 8, 2023 | Version v1
Dataset Open

Supplementary materials for the paper "Towards a self-consistent model of the convective core boundary in upper-main-sequence stars"

Authors/Creators

  • 1. Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany
  • 2. Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany; High-Performance Computing Center Stuttgart, Nobelstraße 19, 70569 Stuttgart, Germany
  • 3. Computer, Computational and Statistical Sciences (CCS) Division and Center for Theoretical Astrophysics (CTA), Los Alamos National Laboratory, Los Alamos, NM 87545, USA
  • 4. Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany; Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120 Heidelberg, Germany
  • 5. Heidelberger Institut für Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany; Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik, Philosophenweg 12, D-69120 Heidelberg, Germany

Description

Supplementary materials for the paper "Towards a self-consistent model of the convective core boundary in upper-main-sequence stars" (Andrassy et al. 2023). The zip files contain the two MESA models used in the paper (one without and one with convective penetration). Files needed to re-compute the models are also included. They work with MESA version 15140.

Files

make_zams.zip

Files (617.7 kB)

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md5:1920f8e53934d2b4bccb799a913b8ac2
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md5:18f6caa3503f448a0792f7541c4618d4
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