Pre-Supernova Structures of Massive Single and Binary-Stripped Stars

A reproduction package for the paper 'Different to the core: the pre-supernova structures of massive single and binary-stripped stars'. It contains inlists for the MESA stellar evolution code and processed output. The author is E. Laplace from the University of Amsterdam.

Use Cases

• Reproduce stellar evolution simulations based on the provided MESA inlists.
• Compare pre-supernova structures of single versus binary-stripped stars based on the processed output.
• Validate new stellar evolution models against the published results.
• Use the inlists as templates for custom MESA simulations of massive stars.

Strengths

• Provides the exact MESA inlists used for the published research, enabling direct reproduction.
• Includes processed output from the simulations, offering a direct comparison point.
• Authored by a researcher at the University of Amsterdam, indicating academic provenance.

Limitations

• Column-level documentation is absent; field semantics must be inferred from the paper or code.
• Row count and dataset size are unknown, which may limit suitability assessment.
• Last update date is unknown; freshness unverified.

Provenance

Source

E. Laplace, University of Amsterdam

Collection Method

Created as a reproduction package for an academic paper.