3D numerical modeling of YSO accretion shocks

3D numerical modeling of YSO accretion shocks

The dynamics of YSO accretion shocks is determined by radiative processes as well as the strength and structure of the magnetic field. A quasi-periodic emission signature is theoretically expected to be observed, but observations do not confirm any such pattern. In this work, we assume a uniform ba...

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Bibliographic Details
Main Authors: Matsakos T., Chièze J.-P., Stehlé C., González M., Ibgui L., de Sá L., Lanz T., Orlando S., Bonito R., Argiroffi C., Reale F., Peres G.
Format: Article
Language:English
Published: EDP Sciences 2014-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136404003

Internet

http://dx.doi.org/10.1051/epjconf/20136404003

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