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- W2015251944 abstract "In dilute astrophysical plasmas, such as planetary nebulae and H II regions, strong lines appear that only have weak, if any, correspondence to the spectrum of laboratory light sources. Some of these are parity forbidden lines, i.e. emission from long-lived metastable states that cannot decay via normal electric dipole (E1) routes but only via the slower M1 and E2 transitions. The long lifetime of the upper levels and their sensitivity to collisions make the lines good diagnostics of the emitting plasma, but then the transition probability, or A-value, of these lines must be known." @default.
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- W2015251944 date "2005-01-01" @default.
- W2015251944 modified "2023-09-25" @default.
- W2015251944 title "Experimental Oscillator Strengths for Forbidden Lines in Complex Spectra" @default.
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- W2015251944 doi "https://doi.org/10.1088/0031-8949/2005/t119/007" @default.
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