144 citations · 520 across the 12 of their papers we have counts for
12 papers
A theoretical investigation of far-infrared fine structure lines at and of the origin of the [OIII]88/[CII]158 enhancement
Camilla T. Nyhagen, Alice Schimek, Claudia Cicone +2
[Abridged] The [OIII]/[CII] and [OIII]/[NII] luminosity ratios have shown to be promising tracers of the ionisation state and gas-phase metall…
Constraining the physical properties of gas in high-z galaxies with far-infrared and submillimetre line ratios
Alice Schimek, Claudia Cicone, Sijing Shen +3
Optical emission line diagnostics, which are a common tool to constrain the properties of the interstellar medium (ISM) of galaxies, become progressively inaccessible at higher red…
Investigating the ultraviolet and infrared radiation through the turbulent life of molecular clouds
Fabio Di Mascia, Andrea Pallottini, Laura Sommovigo +1
Context. Molecular Clouds (MCs) are the place where stars are formed and their feedback starts to take place, regulating the evolution of galaxies. Therefore, MCs represent the cri…
The origin of cold gas in the Circumgalactic Medium
Davide Decataldo, Sijing Shen, Lucio Mayer +2
The presence of cold ( K) gas in the circumgalactic medium (CGM) of galaxies has been confirmed both in observations and high-resolution simulations, but its origi…
High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5
Alice Schimek, Davide Decataldo, Sijing Shen +10
The circumgalactic medium (CGM) is a crucial component of galaxy evolution, but thus far its physical properties are highly unconstrained. As of yet, no cosmological simulation has…
Shaping the structure of a GMC with radiation and winds
D. Decataldo, A. Lupi, A. Ferrara +2
We study the effect of stellar feedback (photodissociation/ionization, radiation pressure and winds) on the evolution of a Giant Molecular Cloud (GMC), by means of a 3D radiative t…
Warm dust in high-z galaxies: origin and implications
L. Sommovigo, A. Ferrara, A. Pallottini +3
ALMA observations have revealed the presence of dust in galaxies in the Epoch of Reionization (redshift ). However, the dust temperature, , remains unconstrained, and thi…
Outflows and extended [CII] halos in high redshift galaxies
Elia Pizzati, Andrea Ferrara, Andrea Pallottini +4
Recent stacked ALMA observations have revealed that normal, star-forming galaxies at are surrounded by extended () [CII] emitting halos which…
A physical model for [CII] line emission from galaxies
A. Ferrara, L. Vallini, A. Pallottini +5
A tight relation between the [CII]158m line luminosity and star formation rate is measured in local galaxies. At high redshift (), though, a much larger scatter is observed…
Deep into the structure of the first galaxies: SERRA views
A. Pallottini, A. Ferrara, D Decataldo +6
We study the formation and evolution of a sample of Lyman Break Galaxies in the Epoch of Reionization by using high-resolution (), cosmological zoom-in simulati…
Photoevaporation of Jeans-unstable molecular clumps
D. Decataldo, A. Pallottini, A. Ferrara +2
We study the photoevaporation of Jeans-unstable molecular clumps by isotropic FUV (6 eV < 13.6 eV) radiation, through 3D radiative transfer hydrodynamical simulations…
Molecular clumps photoevaporation in ionized regions
Davide Decataldo, Andrea Ferrara, Andrea Pallottini +2
We study the photoevaporation of molecular clumps exposed to a UV radiation field including hydrogen-ionizing photons ( eV) produced by massive stars or quasars. We follo…