Cooling and instabilities in colliding flows
Sign Up to like & getrecommendations! Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2577
Abstract: Collisional self-interactions occurring in protostellar jets give rise to strong shocks, the structure of which can be affected by radiative cooling within the flow. To study such colliding flows, we use the AstroBEAR AMR code… read more here.
Keywords: colliding flows; instability; cooling instabilities; instabilities colliding ... See more keywords
Particle acceleration in colliding flows: Binary star winds and other double-shock structures.
Sign Up to like & getrecommendations! Published in 2022 at "Physical review. E"
DOI: 10.1103/physreve.107.025201
Abstract: A shock wave propagating perpendicularly to an ambient magnetic field accelerates particles considerably faster than in the parallel propagation regime. However, the perpendicular acceleration stops after the shock overruns a circular particle orbit. At the… read more here.
Keywords: acceleration colliding; particle acceleration; acceleration; double shock ... See more keywords