112 citations · 187 across the 10 of their papers we have counts for
8 papers · 1 filter
Why is there cold gas inside the Local Bubble?
Tim-Eric Rathjen, Jeffrey L. Linsky
The Local Bubble (LB) extends approximately 100--200~pc from the Sun and contains ~K plasma and warm photoionised gas. Yet the Local Leo Cold Cloud (LLCC) and the Local Ribbo…
SILCC -- IX. The multi-phase interstellar medium at low metallicity
Vittoria Brugaletta, Stefanie Walch, Thorsten Naab +8
The gas-phase metallicity affects heating and cooling processes in the star-forming galactic interstellar medium (ISM) as well as ionising luminosities, wind strengths, and lifetim…
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…
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…
The masses, structure and lifetimes of cold clouds in a high-resolution simulation of a low metallicity starburst
Constantina M. Fotopoulou, Thorsten Naab, Natalia Lahén +6
We present an analysis of the cold gas phase in a low metallicity starburst generated in a high-resolution hydrodynamical simulation of a gas-rich dwarf galaxy merger as part of th…
SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
Tim-Eric Rathjen, Thorsten Naab, Stefanie Walch +3
We present magnetohydrodynamic (MHD) simulations of the star-forming multiphase interstellar medium (ISM) in stratified galactic patches with gas surface densities $Σ_\mathrm{gas}…
CO and [CII] line emission of molecular clouds -- the impact of stellar feedback and non-equilibrium chemistry
S. Ebagezio, D. Seifried, S. Walch +3
We analyse synthetic CO, CO, and [CII] emission maps of simulated molecular clouds of the SILCC-Zoom project, which include an on-the-fly evolution of H, CO, and…
SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
Tim-Eric Rathjen, Thorsten Naab, Philipp Girichidis +6
We present simulations of the multi-phase interstellar medium (ISM) at solar neighbourhood conditions including thermal and non-thermal ISM processes, star cluster formation, and f…