Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1969
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969ap%26ss...4..419r&link_type=abstract
Astrophysics and Space Science, Volume 4, Issue 4, pp.419-426
Astronomy and Astrophysics
Astrophysics
2
Scientific paper
A new exact solution of the macroscopic line transfer equation including electron scattering terms has been obtained for a Milne-Eddington Model atmosphere, and curves of growth based on this solution have been calculated. The results indicate that for lines formed by scattering there is a systematic change in the appropriate theoretical curve of growth as electron scattering becomes an increasingly important source of continuous opacity. In a case where electron scattering is the dominant opacity source, the abundance necessary to produce a given line strength may be decreased by a factor of 2 5 and the derived velocity parameter decreased by 20 30% due to the shifts in the theoretical curves.
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