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The Effect of Binaries on the Chemical Evolution of the Solar Neighbourhood

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 264))

Abstract

We follow the chemical evolution of the solar neighbourhood (the elements He, C, N, O, Ne, Mg, Si, S, Ca and Fe) using a galactic chemical evolutionary code that includes the most recent results of single and binary star evolution. First we discuss the differences in the overall net yields produced seperately by binary and single star evolution for different initial metallicities. Then we implement binary evolution into a galactic code that simulates the chemical evolution of the solar neighbourhood as function of time. Our galactic code makes it possible to study the evolution in time of the rate of the different types of supernovae.

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De Donder, E., Vanbeveren, D. (2001). The Effect of Binaries on the Chemical Evolution of the Solar Neighbourhood. In: Vanbeveren, D. (eds) The Influence of Binaries on Stellar Population Studies. Astrophysics and Space Science Library, vol 264. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9723-4_37

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  • DOI: https://doi.org/10.1007/978-94-015-9723-4_37

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5745-7

  • Online ISBN: 978-94-015-9723-4

  • eBook Packages: Springer Book Archive

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