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Last name: HABART
First name: E.
International audience
International audience
International audience
International audience
The Astrophysical Journal, 614, pp. L129-L132 (2004)
SF2A - Scientific Highlights 2005, eds. F. Casoli, T. Contini, J.-M. Hameury and L. Pagani, EDP Sciences - Conference Series n/a, pp. 421-424 (2006)
Astron. & Astrophys., 449, p. 1067 (2006)
Context. Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about the solid carbon content especially in the planet-forming regions (~0.1–10 au). Fortunately, several refractory carbonaceous species present C-H bonds (such...
Context. Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about the solid carbon content especially in the planet-forming regions (~0.1–10 au). Fortunately, several refractory carbonaceous species present C-H bonds (such...
Context. Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about the solid carbon content especially in the planet-forming regions (~0.1–10 au). Fortunately, several refractory carbonaceous species present C-H bonds (such...