The far-ultraviolet spectrum of Kap CET observed from IUE.
Rego, M.; Fernandez-Figueroa, M. J.; Cornide, M.
Spain
Abstract
A line identification of the spectrum of the G dwarf star Kappa Cet from 1150 to 1950 A, obtained from the IUE satellite in the low resolution mode is presented. The identification of strong emission lines and various absorption lines and their corresponding intensities are indicated. Certain spectral features, such as Si III, 1335 A are suspected to exhibit an absorption core. The emission line Si II 1817 A is remarkably strong.