activity
19982026
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 11.1k across the 121 of their papers we have counts for

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Showing 2012Show all

7 papers · 1 filter

astro-ph.GA2012★ 89 cited

Interstellar matter and star formation in W5-E - A Herschel view

L. Deharveng, A. Zavagno, L. D. Anderson +7

W5-E has been observed with the Herschel-PACS and -SPIRE photometers, at 100, 160, 250, 350, and 500 microns. The dust temperature map shows a rather uniform temperature, in the ra…

astro-ph.GA2012★ 226 cited

The spine of the swan: A Herschel study of the DR21 ridge and filaments in Cygnus X

M. Hennemann, F. Motte, N. Schneider +31

In order to characterise the cloud structures responsible for the formation of high-mass stars, we present Herschel observations of the DR21 environment. Maps of the column density…

astro-ph.SR2012★ 65 cited

The M16 molecular complex under the influence of NGC6611. Herschel's perspective of the heating effect on the Eagle Nebula

T. Hill, F. Motte, P. Didelon +25

We present Herschel images from the HOBYS key program of the Eagle Nebula (M16) in the far-infrared and sub-millimetre, using the PACS and SPIRE cameras at 70μm, 160μm, 250μm, 350μ…

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★ 120 cited

The Dust Properties of Bubble HII Regions as seen by Herschel

L. D. Anderson, A. Zavagno, L. Deharveng +10

Because of their relatively simple morphology, "bubble" HII regions have been instrumental to our understanding of star formation triggered by HII regions. With the far-infrared (F…

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…