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Context.Previous studies have indicated that the 372.4 GHz ground transition of ortho-H2D+ might be a powerful probe of Proto-Planetary Disks. The line could be especially suited for study of the disk mid-plane, where the bulk of the mass resides and where planet formation takes place....

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Detalhes bibliográficos
Auteurs principaux: A. Asensio Ramos, C. Ceccarelli, M. Elitzur
Formato: Article ou chapitre numérique
Idioma:Anglais
Publicado em: EDP Sciences 2007
Assuntos:
Acesso em linha:Accès Université d'Orléans et IFPM
Accès INSA CVL

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