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Published in 2017 at "Atoms"
DOI: 10.3390/atoms5030026
Abstract: Stark broadening parameters are of interest for many problems in astrophysics and laboratory plasmas investigation. Ar II spectral lines are observed in many kinds of stellar atmospheres such as the atmospheres of B-Type stars and…
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Keywords:
lines atmospheres;
subdwarf stars;
atmospheres subdwarf;
widths spectral ... See more keywords