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Magnesium Isotopes in Halo Stars

Astrophysics 2009-06-23 v1

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 = 105^5) Keck HIRES spectra. Unlike previous claims of an important contribution from intermediate-mass AGB stars to the Galactic halo, we find that our 26^{26}Mg/24^{24}Mg ratios can be explained by massive stars.

Keywords

Cite

@article{arxiv.0708.3906,
  title  = {Magnesium Isotopes in Halo Stars},
  author = {Jorge Melendez and Judith G. Cohen},
  journal= {arXiv preprint arXiv:0708.3906},
  year   = {2009}
}

Comments

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

R2 v1 2026-06-21T09:11:41.470Z