activity
19972021
most citedCharacterizing interstellar filaments with Herschel in IC5146

792 citations · 6.6k across the 81 of their papers we have counts for

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Showing 2013Show all

13 papers · 1 filter

astro-ph.GA2013★ 159 cited

Reconstructing the density and temperature structure of prestellar cores from data: A case study for B68 and L1689B

A. Roy, Ph. Andre', P. Palmeirim +22

Utilizing multi-wavelength dust emission maps acquired with , we reconstruct local volume density and dust temperature profiles for the prestellar cores B68 and L1689B us…

astro-ph.GA2013★ 51 cited

Pillars and globules at the edges of H ii regions, Confronting Herschel observations and numerical simulations

P. Tremblin, V. Minier, N. Schneider +24

Pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M16) and the Rosette molecular cloud, and understanding their origin will help ch…

astro-ph.GA2013★ 113 cited

Two Mass Distributions in the L 1641 Molecular Clouds: The Herschel connection of Dense Cores and Filaments in Orion A

D. Polychroni, E. Schisano, D. Elia +23

We present the Herschel Gould Belt survey maps of the L1641 molecular clouds in Orion A. We extracted both the filaments and dense cores in the region. We identified which of dense…

astro-ph.IM2013★ 44 cited

Latest NIKA results and the NIKA-2 project

A. Monfardini, R. Adam, A. Adane +32

NIKA (New IRAM KID Arrays) is a dual-band imaging instrument installed at the IRAM (Institut de RadioAstronomie Millimetrique) 30-meter telescope at Pico Veleta (Spain). Two distin…

astro-ph.GA2013★ 18 cited

The Herschel View of Star Formation

Philippe André

Recent studies of the nearest star-forming clouds of the Galaxy at submillimeter wavelengths with the Herschel Space Observatory have provided us with unprecedented images of the i…

astro-ph.GA2013★ 134 cited

CO outflows from high-mass Class 0 protostars in Cygnus-X

A. Duarte-Cabral, S. Bontemps, F. Motte +3

As natural consequences of the accretion process, outflows are one of the few (indirect) tracers of accretion. We used CO(2-1) PdBI observations towards 6 MDCs in Cygnus-X, contain…