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4 papers · 1 filter
The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
Rebekka Bieri, Thorsten Naab, Sam Geen +3
We introduce the star formation and Supernova (SN) feedback model of the SATIN (Simulating AGNs Through ISM with Non-Equilibrium Effects) project to simulate the evolution of the s…
Constraining the efficiency of cosmic ray acceleration by cluster shocks
F. Vazza, M. Brueggen, D. Wittor +3
We study the acceleration of cosmic rays by collisionless structure formation shocks with ENZO grid simulations. Data from the FERMI satellite enable the use of galaxy clusters as…
Recurrent Novae: Progenitors of SN Ia?
Rolf Walder, Doris Folini, Jean M. Favre +1
We present 3D hydrodynamical simulations of the separated binary RS Ophiuchi (RS Oph), a recurrent nova and potential progenitor of a SN Ia. RS Oph is composed of a red giant (RG)…
Supersonically Turbulent, Shock Bound Interaction Zones
Doris Folini, Rolf Walder, Jean M. Favre
Shock bound interaction zones (SBIZs) are ubiquitous in astrophysics. We present numerical results for 2D and 3D, plane-parallel, infinitely extended SBIZs. Isothermal settings and…