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- W2783208606 abstract "We propose that massive Thorne–Żytkow objects can explode. A Thorne–Żytkow object is a theoretically predicted star that has a neutron core. When nuclear reactions supporting a massive Thorne–Żytkow object terminate, a strong accretion occurs towards the central neutron core. The accretion rate is large enough to sustain a super-Eddington accretion towards the neutron core. The neutron core may collapse to a black hole after a while. A strong large-scale outflow or a jet can be launched from the super-Eddington accretion disc and the collapsing Thorne–Żytkow object can be turned into an explosion. The ejecta have about 10 M⊙ but the explosion energy depends on when the accretion is suppressed. We presume that the explosion energy could be as low as ∼1047 erg and such a low-energy explosion could be observed like a failed supernova. The maximum possible explosion energy is ∼1052 erg and such a high-energy explosion could be observed as an energetic Type II supernova or a superluminous supernova. Explosions of Thorne–Żytkow objects may provide a new path to spread lithium and other heavy elements produced through the irp process such as molybdenum in the Universe." @default.
- W2783208606 created "2018-01-26" @default.
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- W2783208606 date "2018-01-09" @default.
- W2783208606 modified "2023-10-17" @default.
- W2783208606 title "Explosions of Thorne–Żytkow objects" @default.
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- W2783208606 doi "https://doi.org/10.1093/mnrasl/sly005" @default.
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