Astrophysics and Space Science

, Volume 169, Issue 1–2, pp 19–24 | Cite as

Nucleosynthesis in SNIa

  • E. Bravo
  • J. Isern
  • R. Canal
  • J. Labay
Session 1 Stellar Structure and Evolution

Abstract

The final products of a SNIa explosion critically depend on the degree of neutronization of the incinerated material and on the total amount of burned material. Here we study their dependence on the velocity of the burning front and on the density at which the thermonuclear runaway starts. The abundances of54Cr,54, 58Fe,58, 62Ni provide some constraints to the possible values of model parameters.

Keywords

Burning Burning Front Burned Material SNIa Explosion 

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Copyright information

© Kluwer Academic Publishers 1990

Authors and Affiliations

  • E. Bravo
    • 1
    • 4
  • J. Isern
    • 2
    • 4
  • R. Canal
    • 3
    • 4
  • J. Labay
    • 3
    • 4
  1. 1.Departament de Física i Enginyería NuclearUniversitat Politècnica de CatalunyaBarcelonaSpain
  2. 2.Centre d'Estudis AvançatsC.S.I.C.BlanesSpain
  3. 3.Departament de Física de l'Atmosfera, Astronomia i AstrofisicaUniversitat de BarcelonaSpain
  4. 4.Grup d'AstrofisicaInstitut d'Estudis CatalansBarcelonaSpain

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