Modules for Experiments in Stellar Astrophysics (MESA)

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Published April 3, 2018 | Version v2
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Models for paper: Pulsational pair-instability supernovae in very close binaries

Creators

  • 1. CIERA, Northwestern University

Description

Models of pulsational pair-instability supernovae arising from the evolution of metal poor helium stars. These simulations have been made using the MESA code for stellar evolution, and are used in the paper "Pulsational pair-instability supernovae in very close binaries" (to be submitted). Data includes both history and profile files from the simulations, as well as the terminal output and a movie for each.

All MESA output files have been post-processed to reduce their size.

WARNING: This version is modeled with a development MESA version (11123) rather than an official release. 

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