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7 papers · 2 filters
Detection and characterization of a 500 mic dust emissivity excess in the Galactic Plane using Herschel/Hi-GAL observations
D. Paradis, R. Paladini, A. Noriega-Crespo +7
Past and recent observations have revealed unexpected variations in the FIR-mm dust emissivity. In the Herschel spectral range, those are often referred to as a 500μm emission exce…
The Magellanic Mopra Assessment (MAGMA). I. The Molecular Cloud Population of the Large Magellanic Cloud
Tony Wong, Annie Hughes, Jürgen Ott +15
We present the properties of an extensive sample of molecular clouds in the Large Magellanic Cloud (LMC) mapped at 11 pc resolution in the CO(1-0) line. We identify clouds as regio…
Far-Infrared to Millimeter Astrophysical Dust Emission. II: Comparison of the Two-Level Systems (TLS) model with Astronomical Data
D. Paradis, J. -P. Bernard, C. Mény +1
In a previous paper we proposed a new model for the emission by amorphous astronomical dust grains, based on solid-state physics. The model uses a description of the Disordered Cha…
A 100-parsec elliptical and twisted ring of cold and dense molecular clouds revealed by Herschel around the Galactic Center
S. Molinari, J. Bally, A. Noriega-Crespo +38
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-infrared cameras on-board the Herschel satellite, reveal a 3x10^7 solar masses rin…
Spitzer Characterization of Dust in the Ionized Medium of the Large Magellanic Cloud
Deborah Paradis, Roberta Paladini, Alberto Noriega-Crespo +4
A systematic investigation of dust emission associated with the ionized gas has so far been performed only in our Galaxy and for wavelengths longer than 60 μm. Newly available Spit…
Dust Emission from Evolved and Unevolved HII Regions in the Large Magellanic Cloud
C. T. Slater, M. S. Oey, A. Li +8
We present a study of the dust properties of 12 classical and superbubble HII regions in the Large Magellanic Cloud. We use infrared photometry from Spitzer (8, 24, 70, and 160 \mu…