2025 model grid · massive stars

Presupernova models

Presupernova structures and nucleosynthetic yields of non-rotating stars of solar metallicity, with initial masses between 9.22 and 15 M☉.

Published · Limongi et al. 2025, ApJS, 279, 41

Presupernova models

One file per initial mass. [Fe/H] = 0, non rotating.

Initial massFileDownload
9.22 M☉0922a000.pubDownload ↧
10 M☉1000a000.pubDownload ↧
11 M☉1100a000.pubDownload ↧
12 M☉1200a000.pubDownload ↧
13 M☉1300a000.pubDownload ↧
15 M☉1500a000.pubDownload ↧
For the file naming scheme and the meaning of the columns, see the data guide.

Nucleosynthetic yields

Two choices of the mass cut. Yields in solar masses.

For file descriptions and the meaning of the columns, see the yield data guide.

Mass cut from the Burrows et al. (2024) initial mass – 56Ni relation (Ni-Burrows)

Mass cut fixed by the ejection of 0.07 M☉ of 56Ni (Ni-007)

Want a different prescription? Use the interactive yields calculator to choose the mass cut or 56Ni (or a relation with the initial mass), and optionally mixing and fall-back.

Reference

If you use these data, please cite Limongi, M., et al. 2025, ApJS, 279, 41.