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
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
Journal title :
Nuclear physics A