90 citations · 108 across the 4 of their papers we have counts for
4 papers
A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk
Olivier Berné, Emilie Habart, Els Peeters +143
Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiati…
An empirical view of the extended atmosphere and inner envelope of the AGB star R Doradus I. Physical model based on CO lines
T. Khouri, H. Olofsson, W. H. T. Vlemmings +6
The mass loss experienced on the asymptotic giant branch (AGB) at the end of the lives of low- and intermediate-mass stars is widely accepted to rely on radiation pressure acting o…
Formation of the Methyl Cation by Photochemistry in a Protoplanetary Disk
Olivier Berné, Marie-Aline Martin-Drumel, Ilane Schroetter +53
Forty years ago it was proposed that gas phase organic chemistry in the interstellar medium was initiated by the methyl cation CH3+, but hitherto it has not been observed outside t…
The extremely sharp transition between molecular and ionized gas in the Horsehead nebula
C. Hernández-Vera, V. V. Guzmán, J. R. Goicoechea +12
(Abridged) Massive stars can determine the evolution of molecular clouds with their strong ultraviolet (UV) radiation fields. Moreover, UV radiation is relevant in setting the ther…