Physics – Plasma Physics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..401u&link_type=abstract
In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 401-407 (SEE N94-22624 05-75)
Physics
Plasma Physics
Magnetohydrodynamic Flow, Magnetohydrodynamics, Star Formation, Stellar Magnetic Fields, Stellar Models, Computerized Simulation, Herbig-Haro Objects, Interstellar Gas, Magnetic Field Configurations, Molecular Clouds, Plasma Jets, Shock Waves, Stellar Mass Accretion
Scientific paper
The relevance of the magnetic field in the entire process of the star formation is studied. The investigation ranges from the initial contraction from the so called giant molecular cloud in the galaxy to the creation of high speed 'optical jets' in the final stage of star formation in and before the T Tauri stage of the new born stars. The results of magnetohydrodynamic (MHD) simulations made by using a modified MHD code developed for axisymmetric problems, and by using a fourth order accuracy code developed for the upwind total variational diminishing code for the three dimensional astrophysical MHD situations, are reported.
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