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[HTML][HTML] H2 formation on interstellar dust grains: The viewpoints of theory, experiments, models and observations
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 …
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …
The interstellar dust properties of nearby galaxies
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 …
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
We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …
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 …
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 …
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
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 …
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 …
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 …
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
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 …
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 …
formation that include new recipes to track the production and destruction of dust. We …