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D. Paradis

Researcher at University of Toulouse

Publications -  38
Citations -  4921

D. Paradis is an academic researcher from University of Toulouse. The author has contributed to research in topics: Galaxy & Molecular cloud. The author has an hindex of 25, co-authored 36 publications receiving 4593 citations. Previous affiliations of D. Paradis include Centre national de la recherche scientifique & Hoffmann-La Roche.

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Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way

Sergio Molinari, +123 more
TL;DR: In this paper, the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands are presented.
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Hi-GAL: The Herschel Infrared Galactic Plane Survey

Sergio Molinari, +118 more
TL;DR: Hi-GAL as mentioned in this paper is an open-time key project of the Herschel Space Observatory, which aims to detect the earliest phases of the formation of molecular clouds and high-mass stars.
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Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the "dark gas" in our Galaxy

Peter A. R. Ade, +248 more
TL;DR: In this paper, an all sky map of the apparent temperature and optical depth of thermal dust emission is constructed using the Planck-HFI (350μm to 2 mm) and IRAS(100μm) data.
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Planck Early Results: All sky temperature and dust optical depth from Planck and IRAS: Constraints on the "dark gas" in our galaxy

P. A. R. Ade, +205 more
TL;DR: In this paper, the authors constructed an all-sky map of the apparent temperature and optical depth of thermal dust emission using the Planck-HFI and IRAS data and correlated the optical depth maps to tracers of the atomic and molecular gas.
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A 100 pc ELLIPTICAL AND TWISTED RING OF COLD AND DENSE MOLECULAR CLOUDS REVEALED BY HERSCHEL AROUND THE GALACTIC CENTER

TL;DR: In this paper, an elliptical shape having semi-major axes of 100 and 60 pc is deduced, and the major axis of this 100 pc ring is inclined by about 40 degrees with respect to the plane of sky and is oriented perpendicular to the major axes of the Galactic Bar.