pith. sign in

arxiv: 0708.3906 · v1 · submitted 2007-08-29 · 🌌 astro-ph

Magnesium Isotopes in Halo Stars

classification 🌌 astro-ph
keywords halostarshighratiosclaimsclustercontributiondetermined
0
0 comments X
read the original abstract

We have determined Mg isotope ratios in halo field dwarfs and giants in the globular cluster M71 based on high S/N high spectral resolution (R = 10$^5$) Keck HIRES spectra. Unlike previous claims of an important contribution from intermediate-mass AGB stars to the Galactic halo, we find that our $^{26}$Mg/$^{24}$Mg ratios can be explained by massive stars.

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.