[HTML][HTML] H2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations

V Wakelam, E Bron, S Cazaux, F Dulieu, C Gry… - Molecular …, 2017 - Elsevier
Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …

The interstellar dust properties of nearby galaxies

F Galliano, M Galametz, AP Jones - Annual Review of …, 2018 - annualreviews.org
This article gives an overview of the constitution, physical conditions, and observables of
dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial …

Introducing the thesan project: radiation-magnetohydrodynamic simulations of the epoch of reionization

R Kannan, E Garaldi, A Smith, R Pakmor… - Monthly Notices of …, 2022 - academic.oup.com
We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …

The astrodust+ pah model: A unified description of the extinction, emission, and polarization from dust in the diffuse interstellar medium

BS Hensley, BT Draine - The Astrophysical Journal, 2023 - iopscience.iop.org
We present a new model of interstellar dust in which large grains are a single composite
material," astrodust," and nanoparticle-sized grains come in distinct varieties including …

The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

I De Looze, D Cormier, V Lebouteiller… - Astronomy & …, 2014 - aanda.org
Aims. We analyze the applicability of far-infrared fine-structure lines [Cii] 158 μm,[Oi] 63 μm,
and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity …

The dust-to-gas and dust-to-metal ratio in galaxies from z = 0 to 6

Q Li, D Narayanan, R Davé - Monthly Notices of the Royal …, 2019 - academic.oup.com
We present predictions for the evolution of the galaxy dust-to-gas ratio (DGR) and dust-to-
metal ratio (DTM) from z= 0→ 6, using a model for the production, growth, and destruction of …

PHANGS–JWST First Results: Destruction of the PAH Molecules in H ii Regions Probed by JWST and MUSE

OV Egorov, K Kreckel, KM Sandstrom… - The Astrophysical …, 2023 - iopscience.iop.org
Polycyclic aromatic hydrocarbons (PAHs) play a critical role in the reprocessing of stellar
radiation and balancing the heating and cooling processes in the interstellar medium but …

Interstellar polycyclic aromatic hydrocarbon molecules

AGGM Tielens - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
Large polycyclic aromatic hydrocarbon (PAH) molecules carry the infrared (IR) emission
features that dominate the spectra of most galactic and extragalactic sources. This review …

The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

AP Jones, L Fanciullo, M Köhler, L Verstraete… - Astronomy & …, 2013 - aanda.org
Context. The evolution of amorphous hydrocarbon materials, aC (: H), principally resulting
from ultraviolet (UV) photon absorption-induced processing, are likely at the heart of the …

The dust content of galaxies from z = 0 to z = 9

G Pop**, RS Somerville… - Monthly Notices of the …, 2017 - academic.oup.com
We study the dust content of galaxies from z= 0 to z= 9 in semi-analytic models of galaxy
formation that include new recipes to track the production and destruction of dust. We …