Modeling the Progenitor Stars of Observed Type IIP Supernovae
Type IIP supernovae (SNe IIP) are thought to originate from the explosion of massive stars >10 M _⊙ . Their luminosity is primarily powered by the explosion energy and the radioactive decay energy of ^56 Co, with the photosphere location regulated by hydrogen recombination. However, the physical...
| Päätekijät: | , , , , |
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| Aineistotyyppi: | Artikkeli |
| Kieli: | English |
| Julkaistu: |
IOP Publishing
2024-01-01
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| Sarja: | The Astrophysical Journal |
| Aiheet: | |
| Linkit: | https://doi.org/10.3847/1538-4357/ad50c6 |