r-Process Enhanced Halo Stars

Details r-Process Enhanced Halo Stars r-Process Enhanced Halo Stars

2006-10-13

arxiv.org/abs/astro-ph/0610412v1

PoSNIC-IX:014,2006

Astronomy and Astrophysics

Astrophysics

10 pages, 5 figures, To appear in the Proceedings of the International Symposium on Nuclear Astrophysics - Nuclei in the Cosmo

Scientific paper

Abundance observations indicate the presence of rapid-neutron capture (i.e., r-process) elements in old Galactic halo and globular cluster stars. These observations provide insight into the nature of the earliest generations of stars in the Galaxy -- the progenitors of the halo stars -- responsible for neutron-capture synthesis of the heavy elements. The large star-to-star scatter observed in the abundances of neutron-capture element/iron ratios at low metallicities -- which diminishes with increasing metallicity or [Fe/H] -- suggests the formation of these heavy elements (presumably from certain types of supernovae) was rare in the early Galaxy. The stellar abundances also indicate a change from the r-process to the slow neutron capture (i.e., s-) process at higher metallicities in the Galaxy and provide insight into Galactic chemical evolution. Finally, the detection of thorium and uranium in halo and globular cluster stars offers an independent age-dating technique that can put lower limits on the age of the Galaxy, and hence the Universe.

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