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Jet-shaped filamentary ejecta in common envelope evolution

We conduct three-dimensional (3D) hydrodynamical simulations of common envelope evolution (CEE) of a neutron star (NS) that launches jets as it spirals in inside the envelope of a rotating red supergiant (RSG) stellar envelope and find that Rayleigh-Taylor instabilities form filamentary ejecta. We f...

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Bibliografski detalji
Glavni autori: Ron Schreier, Shlomi Hillel, Noam Soker
Format: Artigo
Jezik:Inglês
Izdano: Maynooth Academic Publishing 2025-05-01
Serija:The Open Journal of Astrophysics
Online pristup:https://doi.org/10.33232/001c.138237
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