Computer Science
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kfnt....9...52o&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 9, no. 1, p. 52-55.
Computer Science
Atmospheric Composition, Spectral Line Width, Stellar Atmospheres, Stellar Spectra, Technetium, Atmospheric Models, Calibrating, Metallicity
Scientific paper
Using calibration of the intensity estimates of the Tc I 429.706 nm
line, the equivalent widths of this line were determined for selected
stars. Comparing them with equivalent widths calculated on the basis of
suitable model atmospheres we have obtained the abundances (or abundance
limits) of technetium in the atmospheres of 64 stars of types M, S, C.
Orlov Ya. M.
Shavrina Angelina V.
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