363 citations · 2.7k across the 52 of their papers we have counts for
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Vacuum ultraviolet photolysis of hydrogenated amorphous carbons. III. Diffusion of photo-produced H2 as a function of temperature
Rafael Martín-Doménech, Emmanuel Dartois, Guillermo M. Muñoz Caro
Hydrogenated amorphous carbon (a-C:H) has been proposed as one of the carbonaceous solids detected in the interstellar medium. Energetic processing of the a-C:H particles leads to…
Early Mars volcanic sulfur storage in the cryosphere and formation of transient SO2-rich atmospheres during the Hesperian
F. Schmidt, E. Chassefière, F. Tian +3
In a previous paper (Chassefière et al., Icarus 223, 878-891, 2013), we have shown that most volcanic sulfur released to early Mars atmosphere could have been trapped in the cryosp…
Mantle formation, coagulation and the origin of cloud/core-shine: II. Comparison with observations
N. Ysard, M. Koehler, A. P. Jones +3
Many dense interstellar clouds are observable in emission in the near-IR, commonly referred to as "Cloudshine", and in the mid-IR, the so-called "Coreshine". These C-shine observat…
Mantle formation, coagulation and the origin of cloud/core shine: I. Modelling dust scattering and absorption in the infra-red
A. P. Jones, M. Koehler, N. Ysard +3
Context. The observed cloudshine and coreshine (C-shine) have been explained in terms of grain growth leading to enhanced scatter- ing from clouds in the J, H and K photometric ban…
VUV spectroscopy of carbon dust analogs: contribution to interstellar extinction
L. Gavilan, I. Alata, K. C. Le +3
A full spectral characterization of carbonaceous dust analogs is necessary to understand their potential as carriers of observed astronomical spectral signatures such as the ubiqui…