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Inlists for paper: Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae

<p>MESA (v10108) inlists for the models shown the &quot;Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae&quot; Letter (1903.02135). The inlists reproduce both the single and merger model.</p> <p>Contents:</p> <p>FiducialMergersPPISN.tar.gz</p> <ul> <li>doubleMass</li> <li>evolveMerged</li> <li>evolveSingle</li> <li>preMSmodel</li> <li>README</li> </ul> <p>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.</p> <ul> <li>mergerAtLogTc9.data</li> <li>singleAtLogTc9.data</li> </ul>

ShareScore

36/100

Overall dataset sharing score

Score breakdown

These five areas show where the dataset supports — or may limit — practical reuse.

Stewardship
4
Harmonization
4
Access
16
Reuse readiness
8
Engagement
4