The structure and wavelength of some Pt II lines of astrophysical interest

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Hollow Cathodes, Line Spectra, Peculiar Stars, Platinum, Stellar Atmospheres, Emission Spectra, Fourier Transformation

Scientific paper

Previous studies established the presence of high abundance of platinum in the atmospheres of 'chemically peculiar stars' and a possibility of the presence of nonterrestrial isotope abundances in these stars. This paper presents the detailed information on the structure of 17 Pt II lines of astrophysical importance, including the wavelengths, relative intensities, hyperfine structures, and isotope splittings, measured from high-resolution Fourier transform spectra of a platinum hollow cathode. The probable errors in transition wavenumbers, isotope shifts, and hyperfine splits presented are estimated to be 0.01/cm or less.

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