Nucleosynthesis in Stellar Explosions from Early Stars

Alexander Heger, Stan Woosley, Pamela Vo, Ke-Jung Chen, Candace C Joggerst

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

Abstract

The first generation of stars in the universe may have been different from stars in the present-day universe. They may have been typically more massive than stars that form today, or may have rotated faster and hence their evolution, explosion,and overall nucleosynthesis yield could have been quite different. Theoretical models are needed to qualify and quantify these differences. Here we present nucleosynthesis results from the first generations of stars in the universe and how they may be connected to observed abundance patterns from ultra-metal poor stars.
Original languageEnglish
Title of host publicationAstronomical Society of the Pacific Conference Series
Subtitle of host publicationGalactic Archaeology: Near-Field Cosmology and the Formation of the Milky Way
EditorsWako Aoki, M Ishigaki, T Suda, T Tsujimoto, N Arimoto
Place of PublicationSan Francisco CA USA
PublisherAstronomical Society of the Pacific
Number of pages6
Volume458
ISBN (Electronic)9781583817995
ISBN (Print)9781583817988
Publication statusPublished - 2012

Publication series

NameAstronomical Society of the Pacific Conference Series
PublisherAstronomical Society of the Pacific
Volume458

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