Abstract Stark broadening parameters - full widths at half maximum (FWHM) and shifts for 11 Re II lines have been calculated. The plasma parameters used were electron density of cm−3 and temperature from 5000 K to 80000 K. Calculations were performed using the simplified modified semiempirical (SMSE) approach and compared with calculations by Cowley’s approximative Stark broadening formula at 10000 K, usefull in spectrum synthesis. The results have also been considered in the atmosphere model of A type star and for DB white dwarfs.
On the Stark broadening of the Re II spectral lines
Advances in Space Research ; 71 , 2 ; 1287-1292
2022-07-30
6 pages
Article (Journal)
Electronic Resource
English
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