We use the chemical evolution predictions of cosmological hydrodynamic simulations with
our latest theoretical stellar population synthesis, photoionization, and shock models to …

ABSTRACT A study of gas-phase element abundances reported in the literature for 17
different elements sampled over 243 sight lines in the local part of our Galaxy reveals that …

The physical properties and elemental abundances of the interstellar medium in galaxies
during cosmic reionization are important for understanding the role of galaxies in this …

Aims. Photodissociation by UV light is an important destruction mechanism for carbon
monoxide (CO) in many astrophysical environments, ranging from interstellar clouds to …

A fraction of the dust in the interstellar medium (ISM) enters the heliosphere and is
measured in situ from spacecraft. This review surveys the in situ measurements and …

Cosmic dust particles are small solid objects observed in the solar planetary system and in
many astronomical objects like the surrounding of stars, the interstellar and even the …

Aims. We studied the evolution of the abundance in interstellar dust species that originate in
stellar sources and from condensation in molecular clouds in the local interstellar medium of …

Current emission-line-based estimates of the metallicity of active galactic nuclei (AGN) at
both high and low redshifts indicate that AGN have predominantly solar-to-supersolar …

We introduce a dust model for cosmological simulations implemented in the moving-mesh
code arepo and present a suite of cosmological hydrodynamical zoom-in simulations to …

Earth is constantly bombarded with extraterrestrial dust containing invaluable information
about extraterrestrial processes, such as structure formation by stellar explosions or …