478 citations · 20.2k across the 337 of their papers we have counts for
15 papers · 2 filters
Using CO line ratios to trace the physical properties of molecular clouds
Camilo H. Peñaloza, Paul C. Clark, Simon C. O. Glover +2
The carbon monoxide (CO) rotational transition lines are the most common tracers of molecular gas within giant molecular clouds (MCs). We study the ratio () between CO…
The impact of magnetic fields on the chemical evolution of the supernova-driven ISM
Anabele-Linda Pardi, Philipp Girichidis, Thorsten Naab +7
We present three-dimensional magneto-hydrodynamical simulations of the self-gravitating interstellar medium (ISM) in a periodic (256 pc) box with a mean number density of 0.5 c…
The turbulent life of dust grains in the supernova-driven, multi-phase interstellar medium
Thomas Peters, Svitlana Zhukovska, Thorsten Naab +6
Dust grains are an important component of the interstellar medium (ISM) of galaxies. We present the first direct measurement of the residence times of interstellar dust in the diff…
The SILCC project --- IV. Impact of dissociating and ionising radiation on the interstellar medium and Halpha emission as a tracer of the star formation rate
Thomas Peters, Thorsten Naab, Stefanie Walch +7
We present three-dimensional radiation-hydrodynamical simulations of the impact of stellar winds, photoelectric heating, photodissociating and photoionising radiation, and supernov…
Simulating the formation of massive seed black holes in the early Universe. III: The influence of X-rays
Simon C. O. Glover
The direct collapse black hole (DCBH) model attempts to explain the observed number density of supermassive black holes in the early Universe by positing that they grew from seed b…
TOPoS: III. An ultra iron-poor multiple CEMP system
E. Caffau, P. Bonifacio, M. Spite +15
One of the primary objectives of the TOPoS survey is to search for the most metal-poor stars. Our search has led to the discovery of one of the most iron-poor objects known, SDSS\,…