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Analysis of breit–pauli transition probabilities for lines in o 🇮🇮🇮
Monica Rodriguez
Acceso Abierto
Atribución-NoComercial-SinDerivadas
Atomic data
Atomic processes
Accurate atomic data are essential for understanding the properties of both O 🇮🇮🇮 lines produced by the Bowen fluorescence mechanism and [O 🇮🇮🇮] forbidden lines observed in numerous gaseous nebulae. Improved Breit–Pauli transition probabilities have been published for the carbon sequence. Included were revised data for O 🇮🇮 . The present paper analyzes the accuracy of the data specifically for O 🇮🇮🇮 by comparison with other theory as well as some recent experiments and observations. For the electric dipole transition probabilities, good agreement is found for allowed Bowen fluorescence lines between predictions of intensity ratios with observed data. For forbidden transitions, the Breit–Pauli magnetic dipole transition operator requires corrections that often are neglected. Good agreement is found when these transition probabilities are computed with multiconfiguration Dirac–Hartree–Fock methods.
The Astrophysical Journal
20-09-2009
Artículo
Inglés
Estudiantes
Investigadores
Público en general
Froese Fischer, C., et al., (2009). Analysis of breit–pauli transition probabilities for lines in o 🇮🇮🇮, The Astrophysical Journal. Vol.703(1):500–506
ASTRONOMÍA Y ASTROFÍSICA
Versión aceptada
acceptedVersion - Versión aceptada
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