Abstract

ABSTRACT The spectra of several intermediate and heavy lanthanides, including Ho iii, and Er iii have been positively identified in the spectrum of the silicon star HD 192913. Both the identification of these ions and their occurrence in a silicon star are unusual. These results are discussed in terms of an empirical two-component model of the distribution of lanthanide abundances in Ap stars. Key words: Ap star-lanthanides

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call