Hyperfine splitting of [Al VI] 3.66 mu m and the Al isotopic ratio in NGC 6302

Hyperfine splitting of [Al VI] 3.66 mu m and the Al isotopic ratio in NGC 6302

The core of planetary nebula NGC 6302 is filled with high-excitation photoionized gas at low expansion velocities. It represents a unique astrophysical situation in which to search for hyperfine structure (HFS) in coronal emission lines from highly ionized species. HFS is otherwise blended by therma...

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Detalles Bibliográficos
Autores principales:	Casassus, S, Storey, P, Barlow, M, Roche, P
Formato:	Journal article
Lenguaje:	English
Publicado:	2005

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