Publication Date:
2019-06-27
Description:
The observed strengths of interstellar absorption lines of Fe II and Mn II in the spectra of alpha Vir, beta Cen, pi Sco, and zeta Oph along with laboratory f values of some of these lines between 2343 and 2606 A have been used to determine curves of growth for these ions and the f-values of ten lines of Fe II and three lines of Mn II between 1055 and 1261 A. The Fe and Mn abundances are derived.
Keywords:
SPACE SCIENCES
Type:
Astronomy and Astrophysics; 31; 4, Ap; Apr. 197
Format:
text
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