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Using HST/GHRS Echelle Spectra as Templates for IUE Data Analysis
Published online by Cambridge University Press: 12 April 2016
Abstract
Echelle spectra obtained with the HST/GHRS are used to understand the blending in lower resolution IUE sprectra in the region of the raie ultime line of Au II. Laboratory analysis of the Au II transition has provided an accurate wavelength and transition probability from which the first Au abundances are determined for stars other than the Sun.
- Type
- I. General Properties of CP Stars
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- Copyright © Astronomical Society of the Pacific 1993
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