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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Bibliographic Details
Main Authors: Ron Schreier, Shlomi Hillel, Noam Soker
Format: Article
Language:English
Published: Maynooth Academic Publishing 2025-05-01
Series:The Open Journal of Astrophysics
Online Access:https://doi.org/10.33232/001c.138237
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