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An ever-present snail shell triggered by a dark matter wake
Robert J. J. Grand, Rüdiger Pakmor, Francesca Fragkoudi +5
We utilize a novel numerical technique to model star formation in cosmological simulations of galaxy formation - called Superstars - to simulate a Milky Way-like galaxy with $\gtrs…
Triple evolution: an important channel in the formation of type Ia supernovae
Abinaya Swaruba Rajamuthukumar, Adrian Hamers, Patrick Neunteufel +2
Type Ia supernovae (SNe Ia) are thought to be the result of thermonuclear explosions in white dwarfs (WDs). Commonly considered formation pathways include two merging WDs (the doub…
Close Encounters of Tight Binary Stars with Stellar-mass Black Holes
Taeho Ryu, Rosalba Perna, Ruediger Pakmor +3
Strong dynamical interactions among stars and compact objects are expected in a variety of astrophysical settings, such as star clusters and the disks of active galactic nuclei. Vi…
Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (I) Temporal dependency
Federico G. Iza, Cecilia Scannapieco, Sebastián E. Nuza +5
We use the 30 simulations of the Auriga Project to estimate the temporal dependency of the inflow, outflow and net accretion rates onto the discs of Milky Way-like galaxies. The ne…
The THESAN project: Lyman-alpha emitter luminosity function calibration
Clara Xu, Aaron Smith, Josh Borrow +6
The observability of Lyman-alpha emitting galaxies (LAEs) during the Epoch of Reionization can provide a sensitive probe of the evolving neutral hydrogen gas distribution, thus set…
Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
David J. Whitworth, Rowan J. Smith, Ralf S. Klessen +5
Many studies concluded that magnetic fields suppress star formation in molecular clouds and Milky Way like galaxies. However, most of these studies are based on fully developed fie…