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Contribution of ion to the astrophysical important 471.32 nm He I spectral line broadening
Contribution of ion to the astrophysical important 471.32 nm He I spectral line broadening
2002
Vladimir Milosavljevic
Stevan Djenize
Keywords:
Electron temperature
Nitrogen
Spectral line
Ion
Atomic physics
Molecular physics
Electron density
Chemistry
Correction
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