Modules for Experiments in Stellar Astrophysics (MESA)
Published December 19, 2024 | Version v1
Dataset Open

Spin-down of solar-mass protostars in magnetospheric accretion paradigm

Authors/Creators

  • 1. Osaka University
  • 2. ROR icon National Astronomical Observatory of Japan
  • 3. ROR icon Kurume University
  • 4. The University of Tokyo
  • 5. ROR icon Tohoku University

Description

Supplemental materials for Takasao, Kunitomo, Suzuki, Iwasaki & Tomida (2025, ApJ). The stellar evolution code MESA version 12115 was used to simulate protostellar evolution models. The "Takasao2025.zip" file contains

  1. data/1Msun-HIST-H98.data: our fiducial evolutionary model using the protostellar mass accretion rate in Hartmann et al. (1998)
  2. data/1Msun-HIST-H16.data: an evolutionary model using the accretion rate in Hartmann et al. (2016)
  3. inlists/inlist_simplex_search_controls specifies input parameters
  4. inlists/src/accretion.data specifies the accretion rate
  5. inlists/src/history.inc controls output data in history.data files
  6. ReadMe.md: a ReadMe file

See https://zenodo.org/records/5506424 for the other input flies.

Files

Takasao2025.zip

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