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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…
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…
The end of star formation in Chamaeleon I ? A LABOCA census of starless and protostellar cores
A. Belloche, F. Schuller, B. Parise +7
Chamaeleon I is the most active region in terms of star formation in the Chamaeleon molecular cloud complex. Its population of prestellar and protostellar cores is not known and a…