358 citations · 3.4k across the 48 of their papers we have counts for
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A Corona Australis cloud filament seen in NIR scattered light. III. Modelling and comparison with Herschel sub-millimetre data
M. Juvela, V. -M. Pelkonen, G. J. White +3
With recent Herschel observations, the northern filament of the Corona Australis cloud has now been mapped in a number of bands from 1.2um to 870um. The data set provides a good st…
Isolated starless cores in IRDCs in the Hi-GAL survey
L. A. Wilcock, D. Ward-Thompson, J. M. Kirk +15
In a previous paper we identified cores within infrared dark clouds (IRDCs). We regarded those without embedded sources as the least evolved, and labelled them starless. Here we id…
Cluster-formation in the Rosette molecular cloud at the junctions of filaments
N. Schneider, T. Csengeri, M. Hennemann +31
For many years feedback processes generated by OB-stars in molecular clouds, including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to trigger su…
The Pipe Nebula as seen with Herschel: Formation of filamentary structures by large-scale compression ?
N. Peretto, Ph. Andre, V. Konyves +20
A growing body of evidence indicates that the formation of filaments in interstellar clouds is a key component of the star formation process. In this paper, we present new Herschel…
Cores in Infra-Red Dark Clouds (IRDCs) seen in the Hi-GAL survey between l = 300° and l = 330°
L. A. Wilcock, D. Ward-Thompson, J. M. Kirk +15
We have used data taken as part of the Herschel infrared Galactic Plane survey (Hi-GAL) to study 3171 infrared-dark cloud (IRDC) candidates that were identified in the mid-infrared…