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On the importance of inner-shell transitions for opacity calculations

For high temperatures and densities, stellar opacities obtained from the Opacity Project (OP) were smaller than those obtained from the OPAL project. Iglesias and Rogers [Ap.J. v443, 469 (1995)] suggested that the discrepancy was due to the omission by OP of important atomic inner-shell processes, a...

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Detalles Bibliográficos
Autores principales: Badnell, N R, Seaton, M J
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1088/0953-4075/36/21/015
http://cds.cern.ch/record/639274

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