The challenges of modelling microphysics: ambipolar diffusion, chemistry, and cosmic rays in MHD shocks

Author:

Grassi T123,Padovani M34ORCID,Ramsey J P25ORCID,Galli D4,Vaytet N26,Ercolano B13,Haugbølle T2ORCID

Affiliation:

1. Universitäts-Sternwarte München, Scheinerstr. 1, D-81679 München, Germany

2. Centre for Star and Planet Formation, the Niels Bohr Institute and the Natural History Museum of Denmark, University of Copenhagen, Østervoldgade 5-7, DK-1350 Copenhagen K, Denmark

3. Excellence Cluster Origin and Structure of the Universe, Boltzmannstr. 2, D-85748 Garching bei München, Germany

4. INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy

5. Department of Astronomy, University of Virginia, Charlottesville, VA-22904, USA

6. Data Management and Software Centre, the European Spallation Source ERIC, Ole Maaløes Vej 3, DK-2200 Copenhagen, Denmark

Funder

Horizon 2020

Danish National Research Foundation

German Research Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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