Explosions in Roche-lobe Distorted Stars: Relativistic Bullets in Binaries

Abstract

State-of-the-art surveys reveal that most massive stars in the Universe evolve in close binaries. Massive stars in such systems are expected to develop aspherical envelopes due to tidal interactions and/or rotational effects. Recently, it was shown that point explosions in oblate stars can produce relativistic equatorial ring-like outflows. Moreover, since stripped-envelope stars in binaries can expand enough to fill their Roche lobes anew, it is likely that these stars die with a greater degree of asphericity than the oblate spheroid geometry previously studied. We investigate the effects of this asymmetry by studying the gas dynamics of axisymmetric point explosions in stars in various stages of filling their Roche lobes. We find that point explosions in these pear-shaped stars produce transrelativistic ejecta that coalesce into bullets pointed both toward and away from the binary companion. We present this result and comment on key morphological differences between core-collapse explosions in spherical versus distorted stars in binary systems, effects on gravitational wave sources, and observational signatures that could be used to glean these explosion geometries from current and future surveys.

Strong Bow Shocks: Turbulence and an Exact Self-similar Asymptotic

“…Moreover, this model may also be applicable to runaway supernova (SN) ejecta blobs that outrun the SN shock front and develop bow shocks like what has been observed in the filamentary structures of the Cassiopeia A SN remnant (Fesen et al 2006) or the bidirectional ejecta blobs that might develop from explosions of axisymmetric Roche-lobe distorted Type Ib/c SN progenitors (DuPont et al 2024).…”