activity
20002026
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 7.1k across the 46 of their papers we have counts for

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Showing 2012Show all

7 papers · 1 filter

astro-ph.SR2012★ 595 cited

Herschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?

P. Palmeirim, Ph. André, J. Kirk +23

We present first results from the Herschel Gould Belt survey for the B211/L1495 region in the Taurus molecular cloud. Thanks to their high sensitivity and dynamic range, the Hersch…

astro-ph.SR2012★ 47 cited

Resolving the Vela C ridge with P-ArTeMiS and Herschel

T. Hill, Ph. Andre, D. Arzoumanian +25

We present APEX/P-ArTéMiS 450μm continuum observations of RCW 36 and the adjacent ridge, a high-mass high-column density filamentary structure at the centre of the Vela C molecular…

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.IM2012★ 173 cited

A multi-scale, multi-wavelength source extraction method: getsources

A. Men'shchikov, Ph. André, P. Didelon +3

We present a multi-scale, multi-wavelength source extraction algorithm called getsources. Although it has been designed primarily for use in the far-infrared surveys of Galactic st…

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…