Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 329, Issue 3, Pages 670-674Publisher
OXFORD UNIV PRESS
DOI: 10.1046/j.1365-8711.2002.05011.x
Keywords
hydrodynamics; ISM : jets and outflows; ISM : structure
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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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