• Title of article

    Galactic Chemical Evolution Redux: Atomic Numbers image Original Research Article

  • Author/Authors

    B.K. Gibson، نويسنده , , Y. Fenner، نويسنده , , A. Kiessling، نويسنده ,

  • Issue Information
    هفته نامه با شماره پیاپی سال 2005
  • Pages
    4
  • From page
    259
  • To page
    262
  • Abstract
    Motivated by the inability of Galactic chemical evolution models to reproduce some of the observed solar neighbourhood distribution of elements (and isotopes) with atomic numbers 6⩽Z⩽15, we have revisited the relevant stellar and Galactic models as part of an ambitious new program aimed at resolving these long-standing discrepancies. Avoiding the use of (traditional) parametric models for low- and intermediate-mass stellar evolution, we have generated a new, physically self-consistent, suite of stellar models and integrated the nucleosynthetic outputs into GEtool, our semi-analytical galactic chemical evolution software package. The predicted temporal evolution of several light- and intermediate- mass elements (and their isotopes) in the solar neighbourhood - from carbon to phosphorus - demonstrate the efficacy of the new yields in reconciling theory and observation.
  • Journal title
    Nuclear physics A
  • Serial Year
    2005
  • Journal title
    Nuclear physics A
  • Record number

    1202567