Published October 21, 2021 | Version v1

Numerical Simulations on Cepheus E

Description

With 2D/3D chemo-hydrodynamical (CHD) codes, such as WALKIMYA, we investigate the complex interaction of jets with the protostellar gas, modeling the physical and chemical properties of molecular gas tracers. We show  a comparison between simulations and PdBI observations of the CO emission at arcsec scale which allows us to retrieve the history of the mass loss events that shape the CepE-mm system.

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RO-Poster.pdf

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Additional details

Funding

European Commission
DOC - The Dawn of Organic Chemistry 741002