From the 1 of 6 linked papers with an AI index.
6 papers
Dianoga simulations of galaxy clusters and groups: Properties of the baryonic components
Stefano Borgani, Alice Damiano, Elena Rasia +12
We introduce the Dianoga set of cosmological simulations of galaxy clusters and groups, specifically aimed at studying the impact of the implementation of AGN feedback and star for…
The Drivers of Cosmic Dust Temperature Evolution
Massimiliano Parente, Francesco Salvestrini, Gian Luigi Granato +7
The paper uses a cosmological semi‑analytic galaxy formation model with dust radiative transfer to study how dust temperature evolves with redshift, finding that star‑formation rat…
High [OI] emission lines: ColdSIM simulations and ALMA observations
Massimiliano Parente, Manuela Bischetti, Umberto Maio +8
Neutral-oxygen [OI] far-infrared emission lines at m and m are powerful probes of the physical conditions in the interstellar medium, although they have not been fully…
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…
Galaxy populations of ProtoClusters in cosmological hydrodynamical simulations
Michela Esposito, Stefano Borgani, Veronica Strazzullo +6
The study of protoclusters at cosmic noon is essential to understand the impact on galaxies of the environment and of the transformational processes occurring in this epoch. This w…
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, …