pith. the verified trust layer for science. sign in

arxiv: 0706.3271 · v1 · submitted 2007-06-22 · 🌌 astro-ph

A cool R Coronae Borealis star Z UMi

classification 🌌 astro-ph
keywords starstarsabundanceabundancesanalysedatmosphericborealisconfirmed
0
0 comments X p. Extension
read the original abstract

The high resolution spectra of a R CrB type star Z UMi are analysed. The atmospheric parameters of Z UMi are estimated: Teff=5250+/-250K and log g=0.5+/-0.3. This places Z UMi among the coolest R CrB stars. The hydrogen deficiency of Z UMi is confirmed. The abundances of other elements resemble those found for the minority group of R CrB stars. We note very low iron abundance, [Fe/H]=-1.85, and an excess of lithium, [Li/Fe]=+1.9.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.