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Spatial variation of the cooling lines in the Orion Bar from Herschel/PACS
J. Bernard-Salas, E. Habart, H. Arab +8
We present spatially resolved Herschel/PACS observations of the Orion Bar. We have characterise the emission of the far-infrared fine-structure lines of [CII] (158um), [OI] (63 and…
Herschel Observations of a Potential Core Forming Clump: Perseus B1-E
S. I. Sadavoy, J. Di Francesco, Ph. Andre +17
We present continuum observations of the Perseus B1-E region from the Herschel Gould Belt Survey. These Herschel data reveal a loose grouping of substructures at 160 - 500 micron n…
The Herschel view of massive star formation in G035.39--00.33: Dense and cold filament of W48 undergoing a mini-starburst
Q. Nguyen Luong, F. Motte, M. Hennemann +29
The filament IRDC G035.39--00.33 in the W48 molecular complex is one of the darkest infrared clouds observed by \textit{Spitzer}. It has been observed by the PACS (70 and 160\,$\mi…
Will the starless cores in Chamaeleon I and III turn prestellar?
A. Belloche, B. Parise, F. Schuller +3
The nearby Chamaeleon molecular cloud complex is a good laboratory to study the process of low-mass star formation since it consists of three clouds with very different properties.…
Characterizing interstellar filaments with Herschel in IC5146
D. Arzoumanian, Ph. André, P. Didelon +21
We provide a first look at the results of the Herschel Gould Belt survey toward the IC5146 molecular cloud and present a preliminary analysis of the filamentary structure in this r…
W43: the closest molecular complex of the Galactic Bar?
Q. Nguyen Luong, F. Motte, F. Schuller +9
We used a large database extracted from Galaxy-wide surveys of H {\scriptsize I}, CO 1-0, $8 \micron$ and $870 \micron$ continuum to trace diffuse atomic gas, low- to medium…