24 citations · 68 across the 10 of their papers we have counts for
10 papers
Dust and Grain Size Evolution in Galaxy Simulations: What Matters and What Does Not
Massimiliano Parente, Desika Narayanan, Paul Torrey
We present the first implementation of an evolving dust grain size distribution (GSD) within a semi-analytic cosmological model (SAM) of galaxy evolution. This flexible model self-…
Modeling Dust in Galaxy Evolution Simulations
Massimiliano Parente
Dust grains play a fundamental role in galaxies, influencing both their evolution and observability. As a result, incorporating dust physics into galaxy evolution simulations is es…
Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since
Jakub Nadolny, Michał J. Michałowski, Massimiliano Parente +4
Recent high-redshift () spatially resolved observations with the James Webb Space Telesescope have shown the evolution of the star formation rate (SFR) surface density ($Σ_{\r…
Dust sub-millimetre emission in green valley galaxies
Massimiliano Parente, Cinthia Ragone-Figueroa, Gian Luigi Granato +5
Context. Green valley (GV) galaxies are objects defined on a colour-magnitude diagram, or a colour-mass diagram, as being associated with a transition from a star-forming to a quie…
ACOSMOS: the dust mass function and dust mass density at
A. Traina, B. Magnelli, C. Gruppioni +7
Context. Although dust in galaxies represents only a few percent of the total baryonic mass, it plays a crucial role in the physical processes occurring in galaxies. Studying the d…
Intertwined Formation of , Dust, and Stars in Cosmological Simulations
Cinthia Ragone-Figueroa, Gian Luigi Granato, Massimiliano Parente +4
Context: Molecular hydrogen () is crucial in galaxy formation and evolution, serving as the main fuel for star formation (SF). In metal-enriched environments, …
The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
Jakub Nadolny, Michał J. Michałowski, Massimiliano Parente +6
Removing cold interstellar medium (ISM) from a galaxy is central to quenching star formation. However, the exact mechanism of this process remains unclear. The objective of this wo…
Star Formation and Dust in the Cosmic Web
Massimiliano Parente, Cinthia Ragone-Figueroa, Pablo López +8
The large-scale environment of the cosmic web is believed to impact galaxy evolution, but there is still no consensus regarding the mechanisms. We use a semi-analytic model (SAM) g…
The drop of cosmic dust abundance in a semi-analytic framework
Massimiliano Parente, Cinthia Ragone-Figueroa, Gian Luigi Granato +1
Observations suggest that the amount of galactic dust in the Universe decreased by a factor during the last Gyr. However, cosmological models of galaxy evolutio…
Dust evolution with MUPPI in cosmological volumes
Massimiliano Parente, Cinthia Ragone-Figueroa, Gian Luigi Granato +5
We study the evolution of dust in a cosmological volume using a hydrodynamical simulation in which the dust production is coupled with the MUPPI (MUlti Phase Particle Integrator) s…