Numerical simulations of tail formation in wind interactions with injected material

Details Numerical simulations of tail formation in wind interactions with injected material Numerical simulations of tail formation in wind interactions with injected material

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.329..670f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 329, Issue 3, pp. 670-674.

Astronomy and Astrophysics

Astronomy

18

Hydrodynamics, Ism: Jets And Outflows, Ism: Structure

Scientific paper

A numerical simulation of the interaction of a hypersonic wind with a
mass source shows that, downstream of the source, the injected material
occupies a cone with a sizable opening angle. In contrast, the injected
material is confined to a long, thin tail when the wind is transonic.

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