Hostname: page-component-78c5997874-fbnjt Total loading time: 0 Render date: 2024-11-20T00:57:06.711Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar Nucleosynthesis and Chemical Evolution of Galaxies

Published online by Cambridge University Press:  27 September 2007

M. Busso ,
R.G. Pizzone ,
C. Rolfs ,
C. Spitaleri ,
A. Tumino  and
C. Chiosi
C. Chiosi*
Affiliation:
Department of Astronomy, University of Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
Get access

Abstract

We present the basic theory of nuclear reactions in stars and sketchthe general rules of stellar evolution. Then we shortly review thesubject of supernova explosions both by core collapse in massivestars (type II) and carbon-deflagration in binary systems when oneof the components is a White Dwarf accreting mass from the companion(type Ia). We also present elementary notions of s- and r-processnucleo-synthesis. Finally, we shortly review the topic of galacticchemical evolution and highlight some simple solutions aimed atunderstanding the main observational data on abundances andabundance ratios.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 27: The Third European Summer School on Experimental Nuclear Astrophysics , 2007 , pp. 25 - 39
Copyright
© EAS, EDP Sciences, 2007

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)