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Galactic Chemical Evolution with Rotating Massive Star Yields

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Nuclei in the Cosmos XV

Part of the book series: Springer Proceedings in Physics ((SPPHY,volume 219))

Abstract

I present results from a recent work studying galactic chemical evolution with yields from rotating massive stars; they include, for the first time, the combined effect of metallicity, mass loss and rotation for a large grid of stellar masses and for all stages of stellar evolution. The yields of massive stars are weighted by a metallicity dependent function of the rotational velocities, constrained by observations.

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References

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Author information

Authors and Affiliations

  1. Institut d’Astrophysique de Paris, Sorbonne Université, Paris, France

    Nikos Prantzos

Authors
  1. Nikos Prantzos
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Correspondence to Nikos Prantzos .

Editor information

Editors and Affiliations

  1. Laboratori Nazionali del Gran Sasso, Istituto Nazionale di Fisica Nucleare, L’Aquila, Italy

    Alba Formicola

  2. Laboratori Nazionali del Gran Sasso, Istituto Nazionale di Fisica Nucleare, L’Aquila, Italy

    Matthias Junker

  3. Dipartimento di Matematica e Fisica, Università degli Studi della Campania “Luigi Vanvitelli”, Caserta, Italy

    Lucio Gialanella

  4. Dipartimento di Fisica “E. Pancini”, Università degli Studi di Napoli “Federico II”, Napoli, Italy

    Gianluca Imbriani

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Prantzos, N. (2019). Galactic Chemical Evolution with Rotating Massive Star Yields. In: Formicola, A., Junker, M., Gialanella, L., Imbriani, G. (eds) Nuclei in the Cosmos XV. Springer Proceedings in Physics, vol 219. Springer, Cham. https://doi.org/10.1007/978-3-030-13876-9_14

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