zenodoopen
The stability of massive main-sequence stars as a function of metallicity
<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2012MNRAS.423.3397S">The stability of massive main-sequence stars as a function of metallicity</a></p>
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