Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-27T06:37:13.176Z Has data issue: false hasContentIssue false
  • English
  • Français

Galactic and cosmic chemical evolution with hypernovae

Published online by Cambridge University Press:  23 December 2005

Chiaki Kobayashi
Chiaki Kobayashi
Affiliation:
Max-Planck-Institute for Astrophysics Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss the G-dwarf problem. We finally show the cosmological simulation and discuss the galaxy formation and chemical enrichment.

Keywords

Galaxy: evolutionnucleosynthesis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S228: From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution , May 2005 , pp. 315 - 321
Copyright
© 2005 International Astronomical Union