High Energy Emission from Shocks Due to Jets and Accretion in Young Stars with Disks: Combining Observations, Numerical Models, and Laboratory Experiments - Archive ouverte HAL
Communication Dans Un Congrès Année : 2019

High Energy Emission from Shocks Due to Jets and Accretion in Young Stars with Disks: Combining Observations, Numerical Models, and Laboratory Experiments

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Astrophysique [astro-ph]

Florence Henry  : Connectez-vous pour contacter le contributeur

https://hal.science/hal-03735027

Soumis le : jeudi 21 juillet 2022-11:57:23

Dernière modification le : mercredi 30 octobre 2024-13:07:06

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hal-03735027 , version 1 (21-07-2022)

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R. Bonito, Costanza Argiroffi, Salvatore Orlando, Marco Miceli, Julien Fuchs, et al.. High Energy Emission from Shocks Due to Jets and Accretion in Young Stars with Disks: Combining Observations, Numerical Models, and Laboratory Experiments. JET Simulations, Experiments, and Theory: Ten Years After JETSET. What Is Next?, May 2018, Paris, France, France. pp.49, ⟨10.1007/978-3-030-14128-8_7⟩. ⟨hal-03735027⟩

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