activity
20082017
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 1.9k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2017★ 201 cited

Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()

D. Elia, S. Molinari, E. Schisano +83

Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 m. We present a band-merged catalogue of spatia…

astro-ph.IM2016★ 74 cited

The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission

J. Wei, B. Cordier, S. Antier +77

To take advantage of the astrophysical potential of Gamma-Ray Bursts (GRBs), Chinese and French astrophysicists have engaged the SVOM mission (Space-based multi-band astronomical V…

astro-ph.GA2014★ 26 cited

Characterizing the structure of diffuse emission in Hi-GAL maps

D. Elia, F. Strafella, N. Schneider +18

We present a study of the structure of the Galactic interstellar medium through the Delta-variance technique, related to the power spectrum and the fractal properties of infrared/s…

astro-ph.GA2010★ 1.5k cited

From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Ph. André, A. Men'shchikov, S. Bontemps +54

We summarize the first results from the Gould Belt survey, obtained toward the Aquila Rift and Polaris Flare regions during the 'science demonstration phase' of Herschel. Our 70-50…

astro-ph.GA2010★ 25 cited

Physical properties of the Sh2-104 HII region as seen by Herschel

J. A. Rodón, A. Zavagno, J. -P. Baluteau +46

Context: Sh2-104 is a Galactic H ii region with a bubble morphology, detected at optical and radio wavelengths. It is considered the first observational confirmation of the collect…

astro-ph.GA2010★ 70 cited

The physical properties of the dust in the RCW 120 HII region as seen by Herschel

L. D. Anderson, A. Zavagno, J. A. Rodon +41

Context. RCW 120 is a well-studied, nearby Galactic HII region with ongoing star formation in its surroundings. Previous work has shown that it displays a bubble morphology at mid-…