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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…
Physical properties of high-mass clumps in different stages of evolution
A. Giannetti, J. Brand, A. Sanchez-Monge +6
(Abridged) Aims. To investigate the first stages of the process of high-mass star formation, we selected a sample of massive clumps previously observed with the SEST at 1.2 mm and…
Global collapse of molecular clouds as a formation mechanism for the most massive stars
N. Peretto, G. A. Fuller, A. Duarte-Cabral +8
The relative importance of primordial molecular cloud fragmentation versus large-scale accretion still remains to be assessed in the context of massive core/star formation. Studyin…
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…