activity
20122023
most citedCluster-formation in the Rosette molecular cloud at the junctions of filaments

358 citations · 3.4k across the 48 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2020★ 31 cited

The census of dense cores in the Serpens region from the Herschel Gould Belt Survey

E. Fiorellino, D. Elia, Ph. André +13

The Herschel Gould Belt survey mapped the nearby (d < 500 pc) star-forming regions to understand better how the prestellar phase influences the star formation process. Here we repo…

astro-ph.GA2018★ 212 cited

Characterizing the properties of nearby molecular filaments observed with Herschel

D. Arzoumanian, Ph. André, V. Könyves +8

[Abridged] Molecular filaments have received special attention recently, thanks to new observational results on their properties. In particular, our early analysis of filament prop…

astro-ph.GA2013★ 34 cited

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…

astro-ph.GA2012★ 15 cited

A Corona Australis cloud filament seen in NIR scattered light. III. Modelling and comparison with Herschel sub-millimetre data

M. Juvela, V. -M. Pelkonen, G. J. White +3

With recent Herschel observations, the northern filament of the Corona Australis cloud has now been mapped in a number of bands from 1.2um to 870um. The data set provides a good st…

astro-ph.GA2012★ 13 cited

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…

astro-ph.GA2012★ 358 cited

Cluster-formation in the Rosette molecular cloud at the junctions of filaments

N. Schneider, T. Csengeri, M. Hennemann +31

For many years feedback processes generated by OB-stars in molecular clouds, including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to trigger su…

astro-ph.GA2012★ 134 cited

The Pipe Nebula as seen with Herschel: Formation of filamentary structures by large-scale compression ?

N. Peretto, Ph. Andre, V. Konyves +20

A growing body of evidence indicates that the formation of filaments in interstellar clouds is a key component of the star formation process. In this paper, we present new Herschel…

astro-ph.GA2012

Cores in Infra-Red Dark Clouds (IRDCs) seen in the Hi-GAL survey between l = 300° and l = 330°

L. A. Wilcock, D. Ward-Thompson, J. M. Kirk +15

We have used data taken as part of the Herschel infrared Galactic Plane survey (Hi-GAL) to study 3171 infrared-dark cloud (IRDC) candidates that were identified in the mid-infrared…