Light elements produced by nitrogen-rich type Ic supernovae

Ko Nakamura, Susumu Inoue, Shinya Wanajo, Takeru Suzuki, Toshikazu Shigeyama

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

Abstract

We investigate energetic type Ic supernovae as a production site for 6Li and other light elements in the early stage of the Milky Way.

Original languageEnglish
Title of host publicationAIP Conference Proceedings
Pages446-448
Number of pages3
Volume847
DOIs
Publication statusPublished - 2006
Externally publishedYes
EventORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology - Tokyo
Duration: 2005 Nov 82005 Nov 11

Other

OtherORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology
CityTokyo
Period05/11/805/11/11

Keywords

  • Nuclear reactions, nucleosynthesis, abundances
  • Supernovae; general

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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  • Cite this

    Nakamura, K., Inoue, S., Wanajo, S., Suzuki, T., & Shigeyama, T. (2006). Light elements produced by nitrogen-rich type Ic supernovae. In AIP Conference Proceedings (Vol. 847, pp. 446-448) https://doi.org/10.1063/1.2234454