most citedConnecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants

12 citations · 21 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO2025

Probing the warm dark matter mass with [C II] intensity mapping

Elena Marcuzzo, Cristiano Porciani, Emilio Romano-Díaz +3

The nature of dark matter (DM) is still debated. While cold DM (CDM) is the standard paradigm, warm DM (WDM) may ease some small-scale tensions in the CDM framework. Line-intens…

astro-ph.CO2025★ 1 cited

Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6

Elena Marcuzzo, Cristiano Porciani, Emilio Romano-Díaz +1

Forthcoming measurements of the line-intensity mapping (LIM) power spectrum (PS) are expected to provide valuable constraints on astrophysical and cosmological quantities. We focus…

astro-ph.GA2024

[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST II. CO foreground masking based on an external catalog

C. Karoumpis, B. Magnelli, E. Romano-Díaz +7

Context. The Fred Young Submillimeter Telescope (FYST) line intensity mapping (LIM) survey will measure the power spectrum (PS) of the singly ionized carbon 158 m fine-struc…

astro-ph.GA2024★ 8 cited

HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations

Prachi Khatri, Cristiano Porciani, Emilio Romano-Díaz +2

Aims. We present a new sub-grid model, HYACINTH -- HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations -- for computing the non-equilibrium abundances of…

astro-ph.GA2024★ 12 cited

Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants

Yvonne A. Fichtner, Jonathan Mackey, Luca Grassitelli +2

Energy and momentum feedback from stars is a key element of models for galaxy formation and interstellar medium dynamics, but resolving the relevant length scales to directly inclu…