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On the shape of the mass-function of dense clumps in the Hi-GAL fields. I. SED determination and global properties of the mass-functions
L. Olmi, D. Angles-Alcazar, D. Elia +11
Stars form in dense, dusty clumps of molecular clouds, but little is known about their origin and evolution. In particular, the relationship between the mass distribution of these…
The G305 star-forming complex: Embedded Massive Star Formation Discovered by Herschel Hi-GAL
A. Faimali, M. A. Thompson, L. Hindson +7
We present a Herschel far-infrared study towards the rich massive star- forming complex G305, utilising PACS 70, 160 μm and SPIRE 250, 350, and 500 μm observations from the Hi-GAL…
The spine of the swan: A Herschel study of the DR21 ridge and filaments in Cygnus X
M. Hennemann, F. Motte, N. Schneider +31
In order to characterise the cloud structures responsible for the formation of high-mass stars, we present Herschel observations of the DR21 environment. Maps of the column density…
A multi-wavelength investigation of RCW175: an HII region harboring spinning dust emission
C. T. Tibbs, R. Paladini, M. Compiegne +9
Using infrared, radio continuum and spectral observations, we performed a detailed investigation of the HII region RCW175. We determined that RCW175, which actually consists of two…
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…