The abundance of technetium in stellar atmospheres

Computer Science

Scientific paper

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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.

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