248 citations · 2.3k across the 78 of their papers we have counts for
8 papers · 1 filter
The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations
Alessandro Lupi, Stefano Bovino, Pedro R. Capelo +2
In this study, we present a suite of high-resolution numerical simulations of an isolated galaxy to test a sub-grid framework to consistently follow the formation and dissociation…
The effect of non-equilibrium metal cooling on the interstellar medium
Pedro R. Capelo, Stefano Bovino, Alessandro Lupi +2
By using a novel interface between the modern smoothed particle hydrodynamics code GASOLINE2 and the chemistry package KROME, we follow the hydrodynamical and chemical evolution of…
Fast deuterium fractionation in magnetized and turbulent filaments
Bastian Körtgen, Stefano Bovino, Dominik R. G. Schleicher +4
Deuterium fractionation is considered as an important process to infer the chemical ages of prestellar cores in filaments. We present here the first magneto-hydrodynamical simulati…
Astrochemistry: From primordial gas to present-day clouds
Dominik R. G. Schleicher, Stefano Bovino, Bastian Körtgen +2
Astrochemistry plays a central role during the process of star formation, both in the primordial regime as well as in the present-day Universe. We revisit here the chemistry in bot…
H ortho-to-para conversion on grains: A route to fast deuterium fractionation in dense cloud cores?
Stefano Bovino, Tommaso Grassi, Dominik R. Schleicher +1
Deuterium fractionation, i.e. the enhancement of deuterated species with respect to the non-deuterated ones, is considered to be a reliable chemical clock of star-forming regions.…
The impact of chemistry on the structure of high-z galaxies
A. Pallottini, A. Ferrara, S. Bovino +4
To improve our understanding of high-z galaxies we study the impact of H chemistry on their evolution, morphology and observed properties. We compare two zoom-in high-resolut…
Massive Black Holes from Dissipative Dark Matter
Guido D'Amico, Paolo Panci, Alessandro Lupi +2
We show that a subdominant component of dissipative dark matter resembling the Standard Model can form many intermediate-mass black hole seeds during the first structure formation…
Deuterium fractionation and H2D+ evolution in turbulent and magnetized cloud cores
Bastian Körtgen, Stefano Bovino, Dominik R. G. Schleicher +2
High-mass stars are expected to form from dense prestellar cores. Their precise formation conditions are widely discussed, including their virial condition, which results in slow c…