Characteristic Features of the Spectrum of the Unique roAp Star HD 101065 near the 6708 Å Lithium Resonance Doublet

Details Characteristic Features of the Spectrum of the Unique roAp Star HD 101065 near the 6708 Å Lithium Resonance Doublet Characteristic Features of the Spectrum of the Unique roAp Star HD 101065 near the 6708 Å Lithium Resonance Doublet

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003arep...47..573s&link_type=abstract

Astronomy Reports, vol. 47, Issue 7, p.573-579

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Synthetic spectrum of the peculiar roAp star HD 101065 (Przybylski’s Star) have been computed in the wavelength interval 6705.8 6708.7 Å in order to describe the observed spectrum in the vicinity of the 6708 Å lithium line. Our detailed computations of the synthetic spectrum allowing for the hyperfine structure of the lithium line, lithium isotopic composition, and blending due to lines of rare-earth elements (CeII, NdII, SmII, and others) have yielded estimates of the atmospheric lithium abundance of the star and its 6Li/7Li isotopic ratio.

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