806 citations · 4.1k across the 72 of their papers we have counts for
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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…
Discovery of weak 6.7-GHz CH3OH masers in a sample of high-mass Hi-GAL sources
L. Olmi, E. D. Araya, P. Hofner +4
Maser lines from different molecular species, including water, hydroxyl, and methanol, are common observational phenomena associated with massive star forming regions. In particula…
Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry
Tristan G. Matthews, Peter A. R. Ade, Francesco E. Angilè +29
The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) was created by adding polarimetric capability to the BLAST experiment that was flown in 2003, 20…
Ionization toward the high-mass star-forming region NGC 6334 I
J. L. Morales Ortiz, C. Ceccarelli, D. C. Lis +3
Context. Ionization plays a central role in the gas-phase chemistry of molecular clouds. Since ions are coupled with magnetic fields, which can in turn counteract gravitational col…
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…
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…