On the Origin of Mass Ejection in Failed Supernovae
Some high-mass stars likely end their lives in underluminous implosions that leave behind a black hole, known as failed supernovae. However, neutrinos radiated during proto-neutron-star formation generate a weak (Mach ≳ 1) shock wave in the outer layers of the star, which produces a unique transient...
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| Główni autorzy: | , , |
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| Format: | Artigo |
| Język: | Inglês |
| Wydane: |
IOP Publishing
2026-01-01
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| Seria: | The Astrophysical Journal |
| Hasła przedmiotowe: | |
| Dostęp online: | https://doi.org/10.3847/1538-4357/ae6b85 |
| Etykiety: |
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