Nucleosynthesis in metal-free and metal-poor stars

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

There have been a number of important recent developments in theoretical and observational studies of nucleosyn-thesis, especially regarding nucleosynthetic sources at low metallicities. Those selected for discussion here include the origin of 6Li, the primary production of N, the s-process, and the supernova sources for three groups of metals: (1) C to Zn with mass numbers A<70, (2) Sr to Ag with A∼90-110, and (3) r-process nuclei with A∼130 and above.

Original languageEnglish (US)
Title of host publicationFirst Stars III
Pages283-290
Number of pages8
DOIs
StatePublished - Apr 28 2008
EventFirst Stars III - Santa Fe, NM, United States
Duration: Jul 15 2007Jul 20 2007

Publication series

NameAIP Conference Proceedings
Volume990
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherFirst Stars III
CountryUnited States
CitySanta Fe, NM
Period7/15/077/20/07

Keywords

  • Abundances
  • Neutrinos
  • Nucleosynthesis
  • Supemovae

Fingerprint Dive into the research topics of 'Nucleosynthesis in metal-free and metal-poor stars'. Together they form a unique fingerprint.

Cite this