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Circumstellar disks in high-mass star environments: the early solar system

Published online by Cambridge University Press:  21 October 2010

Thierry Montmerle
Affiliation:
Laboratoire d'Astrophysique de Grenoble, France
Matthieu Gounelle
Affiliation:
Muséum National d'Histoire Naturelle, Paris, France
Georges Meynet
Affiliation:
Observatoire de Genève, Switzerland e-mail: montmerle@obs.ujf-grenoble.fr
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Abstract

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The early solar system represents the only case we have of a circumstellar disk that can be investigated “in situ” -albeit 4.6 Gyr after its formation. Meteorites studies give mounting evidence for an intense irradiation phase of the young circumsolar disk by energetic particles, and also for contamination by products of high-mass stellar and/or explosive nucleosynthesis. We thus discuss the conditions of the birth of the solar system in a high-mass star environment.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

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