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From Prestellar to Protostellar Cores. II. Time Dependence and Deuterium Frac...
International audience -
Discovery of a Superluminal Fe K Echo at the Galactic Center: The Glorious Pa...
We present the result of a study of the X-ray emission from the galactic center (GC) molecular clouds (MCs) within 15 arcmin from Sgr A*. We use XMM-Newton data (about... -
Imaging diffuse clouds: bright and dark gas mapped in CO
23 pages, 22 PostScript figures. Accepted for publication in Astronomy & Astrophysics. Uses aa LaTeX macros. -
Globules and pillars seen in the [CII] 158 micron line with SOFIA
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A detailed view of a molecular cloud in the far outer disk of M 33. Molecular...
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Results of the IRAM M33 Large Program
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The Herschel and JCMT Gould Belt Surveys: Constraining Dust Properties in the...
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Low-velocity shocks traced by extended SiO emission along the W43 ridges: wit...
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The HOBYS Key Program: When Herschel links high-mass star formation to cloud ...
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The Origin of the 6.4 keV Line Emission and H2 Ionization in the Diffuse Mole...
We investigate the origin of the diffuse 6.4 keV line emission recently detected by Suzaku and the source of H2 ionization in the diffuse molecular gas of the Galactic... -
The First Hi-GAL Observations of the Outer Galaxy: A Look at Star Formation i...
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Water ice deuteration: a tracer of the chemical history of protostars
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Low sulfur depletion in the Horsehead PDR
20 pages, 17 figures, accepted in A&A, 2006 June 9 (Figs 1 & 4 are bitmaped) -
Are PAHs precursors of small hydrocarbons in photo-dissociation regions? The ...
16 pages, 10 PostScript figures. In press in Astronomy & Astrophysics. Uses aa LaTeX macros -
Chemical sensitivity to the ratio of the cosmic-ray ionization rates of He an...
Aim: To determine whether or not gas-phase chemical models with homogeneous and time-independent physical conditions explain the many observed molecular abundances in... -
On the potential of the Cherenkov Telescope Array for the study of cosmic-ray...
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Growing evidence for a core formation threshold traced in Herschel Gould Belt...
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Understanding star formation in molecular clouds. I. Effects of line-of-sight...
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The IRAM-30 m line survey of the Horsehead PDR. IV. Comparative chemistry of ...
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The IRAM-30 m line survey of the Horsehead PDR. III. High abundance of comple...
International audience
