164 citations · 453 across the 10 of their papers we have counts for
9 papers
Thermodynamic modeling for numerical simulations based on the generalized cubic equation of state
Theresa Trummler, Martin Glatzle, Alexander Doehring +2
We further elaborate on the generalized formulation for cubic equation of state proposed by Cismondi and Mollerup [Fluid Phase Equilib. 232 (2005)]. With this formulation all well-…
Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
Ivan Kostyuk, Dylan Nelson, Benedetta Ciardi +2
In this work we investigate the dependence of the escape fraction of ionizing photons, , on various galaxy and host halo properties during the epoch of reionization. W…
Radiative transfer of ionizing radiation through gas and dust: grain charging in star forming regions
Martin Glatzle, Luca Graziani, Benedetta Ciardi
The presence of charged dust grains is known to have a profound impact on the physical evolution of the multiphase interstellar medium (ISM). Despite its importance, this process i…
Optical reconstruction of dust in the region of SNR RX J1713.7-3946 from astrometric data
Reimar Leike, Silvia Celli, Alberto Krone-Martins +5
The origin of the radiation observed in the region of the supernova remnant RX J1713.7-3946, one of the brightest TeV emitters, has been debated since its discovery. The existence…
The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
Chris Byrohl, Dylan Nelson, Christoph Behrens +6
Extended Lyman-alpha emission is now commonly detected around high redshift galaxies through stacking and even on individual basis. Despite recent observational advances, the physi…
Resolving nearby dust clouds
R. H. Leike, M. Glatzle, T. A. Enßlin
Aims: Mapping the interstellar medium in 3D provides a wealth of insights into its inner working. The Milky Way is the only galaxy for which detailed 3D mapping can be achieved in…