Karakas, AmandaLattanzio, John2015-12-131323-3580http://hdl.handle.net/1885/76046The chemical evolution of the Universe is governed by the chemical yields from stars, which in turn are determined primarily by the initial stellar mass. Even stars as low as 0.9 M⊙ can, at low metallicity, contribute to the chemical evolution of elemenThe Dawes Review 2: Nucleosynthesis and stellar yields of low-and intermediate-mass single stars201410.1017/pasa.2014.212015-12-11