Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) is the largest
homogeneous high-resolution (∼ 0 farcs 035, or∼ 5 au) disk continuum imaging survey …

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 …

ABSTRACT Spitzer Space Telescope and Herschel Space Observatory imaging of M31 is
used, with a physical dust model, to construct maps of dust surface density, dust-to-gas ratio …

Dust is a ubiquitous feature of the cosmos, impinging directly or indirectly on most fields of
modern astronomy and astrophysics. Dust in the Galactic Environment, Second Edition …

The spatial variations of the gas-to-dust ratio (GDR) provide constraints on the chemical
evolution and lifecycle of dust in galaxies. We examine the relation between dust and gas at …

Aims. The purpose of this work is the characterization of the radial distribution of dust, stars,
gas, and star-formation rate (SFR) in a sub-sample of 18 face-on spiral galaxies extracted …

We present an analysis of the dust and gas in Andromeda, using Herschel images sampling
the entire far-infrared peak. We fit a modified-blackbody model to∼ 4000 quasi-independent …

Context. Analyzing the properties of dust and its evolution in the early phases of star
formation is crucial to put constraints on the collapse and accretion processes as well as on …

The dust properties in the Large and Small Magellanic clouds (LMC/SMC) are studied using
the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500 μm …

Context. Variations in the observed dust emission and extinction indicate a systematic
evolution of grain properties in the transition from the diffuse interstellar medium (ISM) to …