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A multiwavelength study of young massive star forming regions. II. The dust environment
(2007)
We present observations of 1.2 mm dust continuum emission made with the Swedish-ESO Submillimeter Telescope toward 18 luminous IRAS point sources, all with colors typical of compact H II regions and associated with CS(2 ...
THE EARLY STAGES OF STAR FORMATION IN INFRARED DARK CLOUDS: CHARACTERIZING THE CORE DUST PROPERTIES
(The American Astronomical Society, 2010-05-20)
Identified as extinction features against the bright Galactic mid-infrared background, infrared dark clouds (IRDCs)
are thought to harbor the very earliest stages of star and cluster formation. In order to better characterize ...
Polarization in Monte Carlo radiative transfer and dust scattering polarization signatures of spiral galaxies
(EDP Sciences, 2017-05)
Polarization is an important tool to further the understanding of interstellar dust and the sources behind it. In this paper we describe
our implementation of polarization that is due to scattering of light by spherical ...
Discovery of four new massive and dense cold cores
(UNIV CHICAGO PRESS, 2004-07-20)
We report the identification, from a 1.2 mm dust continuum emission survey toward massive star-forming regions, of four strong 1.2 mm sources without counterparts at mid-infrared (Midcourse Space Experiment [MSX]) and ...
VLT spectroscopic analysis of HH 202. Implications on dust destruction and thermal inhomogeneities
(Universidad Nacional Autonoma de Mexico, 2017)
We present a long-slit spectroscopic analysis of Herbig-Haro 202 and the surrounding gas of the Orion Nebula using data from the Very Large Telescope3. We determined the spatial variation of its physical conditions and ...
The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z ~ 4:4 - 5:8
(European Southern Observatory, 2020)
We present dust attenuation properties of spectroscopically confirmed star forming galaxies on the main sequence at a redshift of ∼4.4 − 5.8. Our analyses are based on the far infrared continuum observations of 118 galaxies ...
Attenuation modified by DIG and dust as seen in M31
(IOP Publishing Ltd, 2017)
The spatial distribution of dust in galaxies affects the global attenuation, and hence inferred properties, of galaxies. We trace the spatial distribution of dust in five approximately kiloparsec fields of M31 by comparing ...