activity
20072021
most citedCharacterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTéMiS

102 citations · 216 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2021★ 22 cited

Probing the structure of a massive filament: ArTeMiS 350 and 450 micron mapping of the integral-shaped filament in Orion A

F. Schuller, Ph. André, Y. Shimajiri +18

(abridged) Within the Orion A molecular cloud, the integral-shaped filament (ISF) is a prominent, degree-long structure of dense gas and dust, with clear signs of recent and on-goi…

astro-ph.GA2016★ 102 cited

Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTéMiS

Ph. André, V. Revéret, V. Könyves +28

Herschel observations of nearby molecular clouds suggest that interstellar filaments and prestellar cores represent two fundamental steps in the star formation process. The observa…

astro-ph.IM2014★ 13 cited

The ArTéMiS wide-field submillimeter camera: preliminary on-sky performances at 350 microns

Vincent Reveret, Philippe André, Jean Le Pennec +24

ArTeMiS is a wide-field submillimeter camera operating at three wavelengths simultaneously (200, 350 and 450 microns). A preliminary version of the instrument equipped with the 350…

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.GA2009★ 22 cited

Evidence of triggered star formation in G327.3-0.6. Dust-continuum mapping of an infrared dark cloud with P-ArTéMiS

V. Minier, Ph. André, P. Bergman +17

Aims. Expanding HII regions and propagating shocks are common in the environment of young high-mass star-forming complexes. They can compress a pre-existing molecular cloud and tri…

astro-ph2007★ 10 cited

Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array

Vincent Minier, Gilles Durand, Pierre-Olivier Lagage +4

Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obs…