Magnesium Isotopes in Halo Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Proceedings, First Stars III, July 16-20, 2007, Santa Fe

Scientific paper

10.1063/1.2905536

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.

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