Published July 19, 2021 | Version v1
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Pulsational instability of pre-main sequence models from accretingprotostars I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations

  • 1. University of Innsbruck
  • 2. University of Texas at Austin
  • 3. University of Vienna

Description

MESA and GYRE inlists to reproduce the results of "Pulsational instability of pre-main sequence models from accretingprotostars I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations"

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Is supplement to
arXiv:2107.07568 (arXiv)