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20092024
most citedHerschel view of the Taurus B211/3 filament and striations: Evidence of filamentary growth?

595 citations · 4.3k across the 45 of their papers we have counts for

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Showing 2012Show all

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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★ 80 cited

Profiling filaments: comparing near-infrared extinction and submillimetre data in TMC-1

J. Malinen, M. Juvela, M. G. Rawlings +3

Interstellar filaments are an important part of star formation. To understand the structure of filaments, cross-section profiles are often fitted with Plummer profiles. This profil…

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.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…