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The SIRC team

Our 48 month-long project is proposed by two complementary experimental teams (LERMA, Cergy–Pontoise (surface reactivity) and PIIM, Marseille (bulk ice reactivity)), and one team expert in astrochemical modeling (and observations) (IPAG, Grenoble). The three teams involved in this proposal have been working separately for several years at the forefront of astrochemistry, on the same fundamental topic: How is the molecular richness of our Universe initiated and propagated? Faced with the failure of the present astrochemical models to account for observations, our community believes that only joint efforts of laboratory astrophysics (and especially grain-surface  and quantum chemistry) coupled with simulations and observations will be able to definitively answer to the question.

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PIIM / LAM - Marseille

LERMA - Cergy

SIRC meeting, Paris observatory January 2020

IPAG - Grenoble

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PI : Francois Dulieu,

Emanule  Congiu, Saoud Baouche, Stephan Diana, Laurent Nusbaum,

Shreya Kakkenpara Suresh.

PI : Fabrice Duvernay

Patrice Theulé, Franciele Kruczkiewicz,

Alejandro Gutiérrez, Yohan Layssac

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PI : Cecilia Ceccarelli

Arezu Witzel,

Joan Enrique Romero

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