Breit-Pauli energy levels, transition probabilities, and lifetimes for 3d^5 levels in Fe IV of astrophysical interest

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dc.creatorFischer, Charlotte Froese
dc.creatorRubin, Robert H.
dc.date2004-08-24
dc.date.accessioned2026-07-07T02:14:21Z
dc.date.available2026-07-07T02:14:21Z
dc.descriptionEnergy levels, lifetimes, and transition probabilities for transitions between computed levels of 3d^5 of Fe IV are reported. The E2 and M1 transition probabilities are compared with earlier theoretical results, often only the values published by Garstang in 1958. From the available astronomical observations of optical emission lines arising from the same level, a few direct tests are now possible and they show consistency with the theoretical calculations.
dc.descriptionMNRAS accepted; 20 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0408423
dc.identifierhttp://arxiv.org/abs/astro-ph/0408423
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8081
dc.subjectAstrophysics
dc.titleBreit-Pauli energy levels, transition probabilities, and lifetimes for 3d^5 levels in Fe IV of astrophysical interest
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