RMxAA

Revista Mexicana de Astronomía y Astrofísica

ISSN: 3061-8649
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Keywords

HYDRODYNAMICS
ISM
JETS AND OUTFLOWS
SHOCK

How to Cite

A Comparison Between Analytic and Numerical Results of a Steady Jet Model. (1993). Revista Mexicana De Astronomía Y Astrofísica, 25(1), 95. https://astronomia.unam.mx/journals/rmxaa/article/view/1993rmxaa..25...95b

Abstract

The structures of well aligned knots in stellar jets can be interpreted in terms of crossing shock models. In this paper, new analytic and numerical niodds for the formation of crossing shocks in steady jets are presented. The good agreement ibund between analytic and numerical results allows us to present clear predictions of the properties of steady crossing shocks as a flinction of the flow parameters. These predictions should be useful for trying to identif the crossing shock structures that possibly exist in stellar jets.
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