True Pair-instability Supernova Descendant: Implications for the First Stars’ Mass Distribution
The initial mass function (IMF) of the first Population III (Pop III) stars remains a persistent mystery. Their predicted massive nature implies the existence of stars exploding as pair-instability supernovae (PISNe), but no observational evidence had been found. Now, the LAMOST survey claims to hav...
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| Hoofdauteurs: | , , |
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| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
IOP Publishing
2024-01-01
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| Reeks: | The Astrophysical Journal Letters |
| Onderwerpen: | |
| Online toegang: | https://doi.org/10.3847/2041-8213/ad2466 |
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