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Chemical Enrichment of the First Binaries

Published online by Cambridge University Press:  17 August 2016

Ke-Jung Chen
Ke-Jung Chen*
Affiliation:
Division of Theoretical Astronomy, National Astronomical Observatory of Japan, Tokyo, Japan Department of Astronomy & Astrophysics, University of California, Santa Cruz, California, USA
*
*EACOA Fellow, email: ken.chen@nao.ac.jp
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Abstract

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Recent studies of Population III (Pop III) star formation suggest that the primordial star-forming clouds can fragment to form binary or multiple stellar systems inside dark matter minihalos. Here, we briefly present the chemical enrichment of the Pop III binary scenarios.

Keywords

stars: formation – stars: Population III – galaxies: formation – early universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 6
Copyright
Copyright © International Astronomical Union 2016 

References

Chen, K.-J., Bromm, V., Heger, A., Jeon, M., & Woosley, S. 2015, ApJ, 802, 13 CrossRefGoogle Scholar