I11: COR2DISC, des cœurs pré-stellaires aux disques proto-planétaires

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  • Traduction en cours

    Understanding star and planet formation is one of the major goal in modern astrophysics and must now be tackled using a multidisciplinary approach. Here we propose to combine star formation numerical simulations of cloud collapse with microphysical evolution gas and dust models to understand how material from the Interstellar Medium (ISM) is delivered into a protoplanetary disc, such as the solar nebula. Confrontations to meteoritic and specraft data thanks to the coupling of ISM simulations with solar nebula disc models will trigger important progress for our knowledge of the coupling between ISM and planet formation.



    WP Leader : Patrick Hennebelle – AIM/IPGP



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