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20242026
most citedSimulating nearby disc galaxies on the main star formation sequence II. The gas structure transition in low and high stellar mass discs

3 citations · 8 across the 5 of their papers we have counts for

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5 papers · 1 filter

astro-ph.GA20261 cited

Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability

Chaitra, Antonio Ragagnin, Milena Valentini +3

Cosmological hydrodynamical simulations are powerful tools for studying galaxy formation, yet their predictive precision is limited by stochastic variability and numerical uncertai…

astro-ph.GA20251 cited

Dynamical friction and massive black hole orbits: analytical predictions and numerical solutions

Alice Damiano, Stefano Borgani, Milena Valentini +4

We investigate the orbital decay of a massive BH embedded in a dark matter halo and a stellar bulge, using both analytical and numerical simulations with the aim of developing and…

astro-ph.GA20253 cited

Simulating nearby disc galaxies on the main star formation sequence II. The gas structure transition in low and high stellar mass discs

Pierrick Verwilghen, Eric Emsellem, Florent Renaud +14

Recent hydrodynamical simulations of isolated barred disc galaxies have suggested a structural change in the distribution of the interstellar medium (ISM) around a stellar mass M$_…

astro-ph.GA20251 cited

Multi-wavelength properties of LISA detectable events

Srija Chakraborty, Simona Gallerani, Fabio Di Mascia +5

We investigate the intrinsic and observational properties of galaxies hosting coalescing massive black holes (MBHs) that gives rise to gravitational waves (GWs) detect…

astro-ph.GA2024

Is GN-z11 powered by a super-Eddington massive black hole?

Maulik Bhatt, Simona Gallerani, Andrea Ferrara +6

Observations of quasars powered by supermassive black holes (SMBHs; ) challenge our current understanding of early black hole (BH) f…