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The EASE Scenario: Dynamical Study of the Supernova Phase

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The First Stars

Part of the book series: ESO ASTROPHYSICS SYMPOSIA ((ESO))

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Abstract.

We revisit the most often encountered argument against self-enrichment in globular clusters, namely the ability of a few number of supernovae to disrupt the proto-globular cloud. We show that, within the context of the Fall and Rees theory, primordial proto-globular cluster clouds may sustain several hundreds of Type II supernovae. Furthermore, the corresponding self-enrichment level is in agreement with galactic halo globular cluster metallicities.

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Authors and Affiliations

  1. Institute of Astrophysics and Geophysics, University of Liège, Belgium

    Geneviève Parmentier, Emannuel Jehin, Pierre Magain, Arlette Noels & Anne Thoul

Authors
  1. Geneviève Parmentier
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  2. Emannuel Jehin
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  3. Pierre Magain
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  4. Arlette Noels
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  5. Anne Thoul
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Achim Weiss Tom G. Abel Vanessa Hill

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Parmentier, G., Jehin, E., Magain, P., Noels, A., Thoul, A. The EASE Scenario: Dynamical Study of the Supernova Phase. In: Weiss, A., Abel, T.G., Hill, V. (eds) The First Stars. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10719504_36

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  • DOI: https://doi.org/10.1007/10719504_36

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-67222-7

  • Online ISBN: 978-3-540-46461-7

  • eBook Packages: Springer Book Archive

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