Documentation scienceplus.abes.fr version Bêta

À propos de : Elemental abundance studies of CP stars        

AttributsValeurs
type
Is Part Of
Subject
subtitle
  • III. The magnetic CP stars α Scl and HD 170973
Title
  • Elemental abundance studies of CP stars
Date
has manifestation of work
related by
Author
Abstract
  • Fine analyses of the magnetic CP stars α Scl and HD 170973 are presented using ATLAS9 model atmospheres which have same bulk metallicity as the deduced abundances. The light elements are mostly solar except for silicon, and all the heavier elements except nickel in HD 170973, which is solar, are greatly overabundant. The iron peak elements are typically 10 times overabundant, Sr is of order of 1000 times solar, Y and Zr are of order of 100 times solar. The rare earths are 1000 or more times overabundant.
article type
publisher identifier
  • aa10362
Date Copyrighted
Rights
  • © ESO, 2001
Rights Holder
  • ESO
is part of this journal
is primary topic of



Alternative Linked Data Documents: ODE     Content Formats:       RDF       ODATA       Microdata