MHD numerical simulations of proto-stellar jets

Details MHD numerical simulations of proto-stellar jets MHD numerical simulations of proto-stellar jets

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ssrv..107..337c&link_type=abstract

Space Science Reviews, v. 107, Issue 1, p. 337-340 (2003).

Physics

1

Herbig-Haro Objects, Magnetohydrodynamics, Numerical Technique, Stellar Formation

Scientific paper

We will summarize in this paper the effects that the presence of the
magnetic field can cause to proto-stellar jet dynamics, structure and
emission line properties, and the differences between two- and
three-dimensional numerical simulations will be emphasized.

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