$^{56}$Ni production in long-lived binary neutron star merger remnants

Fuente: arXiv

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Dettagli Bibliografici
Autori principali:	Jacobi, Maximilian, Magistrelli, Fabio, Loffredo, Eleonora, Ricigliano, Giacomo, Chiesa, Leonardo, Bernuzzi, Sebastiano, Perego, Albino, Arcones, Almudena
Natura:	Preprint
Pubblicazione:	2025
Soggetti:	High Energy Astrophysical Phenomena
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

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