270 citations · 920 across the 13 of their papers we have counts for
22 papers
On the typical width of Herschel filaments
Ph. André, P. Palmeirim, D. Arzoumanian
Herschel studies suggest that nearby (d < 500 pc) molecular filaments have a typical half-power width ~0.1pc, but this finding has been questioned on the ground that the measured w…
Filament coalescence and hub structure in MonR2: Implications to massive star and cluster formation
M. S. N. Kumar, D. Arzoumanian, A. Men'shchikov +3
Here we study the MonR2 star forming region, which has a rich network of filaments joining in a star cluster forming hub, aiming at understanding the hub structure and to examine t…
Probing the structure of a massive filament: ArTeMiS 350 and 450 micron mapping of the integral-shaped filament in Orion A
F. Schuller, Ph. André, Y. Shimajiri +18
(abridged) Within the Orion A molecular cloud, the integral-shaped filament (ISF) is a prominent, degree-long structure of dense gas and dust, with clear signs of recent and on-goi…
The Hi-GAL compact source catalogue -- II. The 360° catalogue of clump physical properties
D. Elia, M. Merello, S. Molinari +29
We present the catalogue of physical properties of Hi-GAL compact sources, detected between 70 and 500 m. This release not only completes the analogous catalogue pre…
Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations
S. Pezzuto, M. Benedettini, J. Di Francesco +20
(Abridged) In this paper, we present analyses of images taken with the Herschel ESA satellite from 70mu to 500mu. We first constructed column density and dust temperature maps. Nex…
Compressed magnetized shells of atomic gas and the formation of the Corona Australis molecular cloud
Andrea Bracco, David Bresnahan, Pedro Palmeirim +4
We present the identification of the previously unnoticed physical association between the Corona Australis molecular cloud (CrA), traced by interstellar dust emission, and two she…