H
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....
Guardado en:
| Autores principales: | , , |
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| Formato: | Article ou chapitre numérique |
| Lenguaje: | Anglais |
| Publicado: |
EDP Sciences
2007
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| Materias: | |
| Acceso en línea: | Accès Université d'Orléans et IFPM Accès INSA CVL |