Proceedings of IAU S228 detailing progress in our knowledge of element production and evolution.The solutions suggested for the solar neighbourhood aquot;G-dwarf problemaquot; include 1) gas infall. ... As we have shown in our Subaru/HDS observation of the Ursa Minor dSph, the stars in dSph galaxies show different distributions in the ... [a/Fe] of the member stars with [Fe/H] alt; a2 are higher than the solar abundance ratios, and [a/Fe] approach the solar value as Fc/H] increases at [Fe/H] agt; -2 (Tolstoy ( 2005)anbsp;...
|Title||:||From Lithium to Uranium (IAU S228)|
|Author||:||International Astronomical Union. Symposium, Vanessa Hill, Patrick Francois, Francesca Primas|
|Publisher||:||Cambridge University Press - 2005|