activity
20152026
most citedStarBench: The D-type expansion of an HII region

99 citations · 141 across the 13 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

astro-ph.GA2024★ 3 cited

The origin and evolution of the [CII] deficit in HII regions and star-forming molecular clouds

Stefano Ebagezio, Daniel Seifried, Stefanie Walch +1

We analyse synthetic maps of the [CII] 158 m line and FIR continuum of simulated molecular clouds (MCs) within the SILCC-Zoom project to study the origin of the [CII] deficit, i…

astro-ph.GA2024★ 6 cited

The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium

Vittoria Brugaletta, Stefanie Walch, Thorsten Naab +6

Low-metallicity environments are subject to inefficient cooling. They also have low dust-to-gas ratios and therefore less efficient photoelectric (PE) heating than in solar-neighbo…

astro-ph.GA2024★ 2 cited

SILCC -- VIII: The impact of far-ultraviolet radiation on star formation and the interstellar medium

Tim-Eric Rathjen, Stefanie Walch, Thorsten Naab +4

We present magnetohydrodynamic simulations of star formation in the multiphase interstellar medium to quantify the impact of non-ionising far-ultraviolet (FUV) radiation within the…

astro-ph.GA2024

The Molecular Cloud Lifecycle I: Constraining H2 formation and dissociation rates with observations

Shmuel Bialy, Blakesley Burkhart, Daniel Seifried +9

Molecular clouds (MCs) are the birthplaces of new stars in galaxies. A key component of MCs are photodissociation regions (PDRs), where far-ultraviolet radiation plays a crucial ro…

astro-ph.GA2024

The Molecular Cloud Lifecycle II: Formation and Destruction of Molecular Clouds Diagnosed via H Fluorescent Emission Emission

Blakesley Burkhart, Shmuel Bialy, Daniel Seifried +11

Molecular hydrogen (H) formation and dissociation are key processes that drive the gas lifecycle in galaxies. Using the SImulating the LifeCycle of Molecular Clouds (SILCC) zoo…