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Observatoire Midi-Pyrénés, UMR 5562 CNRS, Laboratoire Dynamique Terrestre et Planétaire, Université Paul Sabatier, Toulouse III, Toulouse, France
Laboratoire Dynamique Terrestre et Planetaire, CNRS, Univ. P. Sabatier, Observatoire Midi-Pyrenees, Toulouse, France
A Surface Dissolution/Precipitation Model for the Development of Lakes on Titan, Based on an Arid Terrestrial Analogue: The Pans and Calcretes of Etosha (Namibia)
Formation of Titan's Lakes by Episodic Dissolution and Precipitation of a Surface Layer Under Semi-Arid Conditions: Comparison with the Pans and Calcretes of Etosha (Namibia)
Minor Planet Observations [I79 AstroCamp, Nerpio]
Thermal analysis of fractures at Cerberus Fossae, Mars: Detection of air convection in the porous debris apron
What Does Control the Thermal Behaviour of the Pits Near Arsia Mons?
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