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On the shape of the mass-function of dense clumps in the Hi-GAL fields. II. Using Bayesian inference to study the clump mass function
L. Olmi, D. Angles-Alcazar, D. Elia +6
Context. Stars form in dense, dusty clumps of molecular clouds, but little is known about their origin, their evolution and their detailed physical properties. In particular, the r…
Two Mass Distributions in the L 1641 Molecular Clouds: The Herschel connection of Dense Cores and Filaments in Orion A
D. Polychroni, E. Schisano, D. Elia +23
We present the Herschel Gould Belt survey maps of the L1641 molecular clouds in Orion A. We extracted both the filaments and dense cores in the region. We identified which of dense…
The first Hi-GAL observations of the outer Galaxy: a look to star formation in the third Galactic quadrant in the longitude range 216.5 < l < 225.5
D. Elia, S. Molinari, Y. Fukui +17
We present the first Herschel PACS and SPIRE photometric observations in a portion of the outer Galaxy ( and $-2^{\circ} \lesssi…
First results from the Herschel Gould Belt Survey in Taurus
J. M. Kirk, D. Ward-Thompson, P. Palmeirim +26
The whole of the Taurus region (a total area of 52 sq. deg.) has been observed by the Herschel SPIRE and PACS instruments at wavelengths of 70, 160, 250, 350 and 500 μm as part of…
A Hi-GAL study of the high-mass star-forming region G29.96-0.02
M. T. Beltran, L. Olmi, R. Cesaroni +9
Context. G29.96-0.02 is a high-mass star-forming cloud observed at 70, 160, 250, 350, and 500 microns as part of the Herschel survey of the Galactic Plane during the Science Demons…