Published April 17, 2019 | Version 1.0
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Inlists for paper: Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae

  • 1. University of Birmingham
  • 2. University of Chinese Academy of Sciences
  • 3. Monash University
  • 4. University of Amsterdam
  • 5. Oxford University

Description

MESA (v10108) inlists for the models shown the "Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae" Letter (1903.02135). The inlists reproduce both the single and merger model.

Contents:

FiducialMergersPPISN.tar.gz

  • doubleMass
  • evolveMerged
  • evolveSingle
  • preMSmodel
  • README

We also attach the single and merger MESA models at the moment where the central temperature is close to 10^9 K. These models where used to estimate the properties of the star, particularly core and envelope masses, as well as element abundances.

  • mergerAtLogTc9.data
  • singleAtLogTc9.data

Files

Files (24.6 MB)

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md5:b6a3959baaf0e01abcbd9e4a6e99767b
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md5:d3cff9d4c7faf422d70e5c36c5ca400c
13.6 MB Download
md5:ce6eccb5d2d005cfd4cd27e6246cfe49
10.9 MB Download