collaborators

6 papers

astro-ph.SR2026

High mass accretion rates onto evolved stripped-envelope massive stars by jet-induced mass removal

Yotham Cohen, Ealeal Bear, Noam Soker

Simulating one-dimensional stellar evolution models with MESA, we show that removing the outer inflated envelope of a mass-accreting evolved stripped-envelope star, like a Wolf-Ray…

astro-ph.SR2025

Jet-Driven Formation of Bipolar Rings in Planetary Nebulae: Numerical Simulations Inspired by NGC 1514

Muhammad Akashi, Ealeal Bear, Noam Soker

We conduct three-dimensional hydrodynamical simulations of jets launched into a dense shell, reproducing two rings in a bipolar structure that resemble the two dusty rings of the p…

astro-ph.HE2025

Natal kick by early-asymmetrical pairs of jets to the neutron star of supernova remnant S147

Dmitry Shishkin, Ealeal Bear, Noam Soker

We analyze the bipolar morphology of the jet-shaped core-collapse supernova (CCSN) remnant (CCSNR) S147 and its neutron star (NS) kick velocity, and suggest that two pairs of unequ…

astro-ph.HE2025

The Puppis A supernova remnant: an early jet-driven neutron star kick followed by jittering jets

Ealeal Bear, Dmitry Shishkin, Noam Soker

We identify a point-symmetric morphology of three pairs of ears/clumps in the core-collapse supernova remnant (CCSNR) Puppis A, supporting the jittering jets explosion mechanism (J…

astro-ph.SR2025

Enabling high mass accretion rates onto massive main sequence stars by outer envelope mass removal

Ariel Scolnic, Ealeal Bear, Noam Soker

Using the one-dimensional numerical code MESA, we simulate mass accretion at very high rates onto massive main sequence stars, M=30, 60, 80 Mo, and find that these stars can accret…

astro-ph.SR2025

On the response of massive main sequence stars to mass accretion and outflow at high rates

Ealeal Bear, Noam Soker

With a one-dimensional stellar evolution model, we find that massive main-sequence stars can accrete mass at very high mass accretion rates without expanding much if they lose a si…