Inlists for paper: Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae
<p>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.</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