7 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-…
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…
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, MichaÅ J. MichaÅowski, 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_{\…
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, …
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…