Magnesium Isotopes in Halo Stars
arXiv:0708.3906 · doi:10.1063/1.2905536
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.
Proceedings, First Stars III, July 16-20, 2007, Santa Fe