Abstract
AbstractRecent determinations of abundances of heavy elements in CP stars are examined. An emphasis is placed on those elements which are found in a group of CP Stars but not in others. Fragmentary data are available for most of heavy elements. Systematic surveys (especially in the UV region) using a large sample of stars are needed before we understand the physics of the apparently erratic behavior of heavy elements in CP stars.
Publisher
Cambridge University Press (CUP)