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  • Introduction

  • The stellar life cycle

    • How stars grow old: H- and He-core burning
    • The nuclear cauldron and high mass loss: the AGB phase
    • Retirement party: colorful nebulae and unexpected turns

  • Nuclear production of elements

    • The physical model
    • Carbon and heavy elements beyond iron (the s-process)

  • Summary and Conclusions

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Last updated: January 29, 2014

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