Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

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 …

ABSTRACT ALMA observations have revealed the presence of dust in the first generations
of galaxies in the Universe. However, the dust temperature T d remains mostly …

Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is
required when converting (sub) millimetre broad-band flux to total infrared luminosity (L IR) …

We present subkiloparsec-scale mapping of the 870 μm ALMA continuum emission in six
luminous (L IR∼ 5× 10 12 L⊙) submillimeter galaxies (SMGs) from the ALESS survey of the …

THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G): PRECISE STELLAR
MASS DISTRIBUTIONS FROM AUTOMATED DUST CORRECTION AT 3.6 μm - IOPscience …

ABSTRACT The Dwarf Galaxy Survey (DGS) program is studying low-metallicity galaxies
using 230 hr of far-infrared (FIR) and submillimetre (submm) photometric and spectroscopic …

Aims. Within the framework of the DustPedia project we investigate the properties of cosmic
dust and its interaction with stellar radiation (originating from different stellar populations) for …

We report new polarimetric and photometric maps of the massive star-forming region OMC-1
using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy. We …

Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: The KINGFISH
Sample - IOPscience This site uses cookies. By continuing to use this site you agree to our use …