We conclude that if stellar abundances with precisions of 0.01–0.03 dex is usually reached in studies of additional distant stars and stars on the enormous and supergiant branches, numerous far more fascinating potential applications, of wonderful relevance to stellar and galaxy evolution, are possible. Consequently, in scheduling abundance surveys, it https://felixrutut.worldblogged.com/38729772/the-stellar-abundance-for-dummies