Abstract
Abstract
Thulium abundance is unknown in the atmospheres of low and medium-mass evolved stars. The reason is the weakness of lines and the crowded spectra. We examined the spectra of two late-type stars in a broad wavelength region to search for thulium lines. Thulium abundance was estimated in the atmospheres of barium star HD 204075 and post-asymptotic giant branch star HD 235858 for the first time,
log
ϵ
(
Tm
)
≃
0.1
and ≲1.3, respectively.
Publisher
American Astronomical Society
Cited by
1 articles.
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