Jets

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Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..119f&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 119-125

Astronomy and Astrophysics

Astrophysics

Gas Dynamics, Herbig-Haro Objects, Magnetohydrodynamic Flow, Magnetohydrodynamic Stability, Molecular Gases, Plasma Interactions, Plasma Jets, Shock Wave Interaction, Stellar Models, Bernoulli Theorem, Burger Equation, Plasma Temperature, Shock Waves

Scientific paper

Despite its title, this paper is mainly concerned with some of the latest theoretical work on the Herbig-Haro (HH) objects associated with stellar jets. Recent measurements of the proper motions of HH objects show that even those near the source are moving at about the same speed as the jet fluid. This means that they cannot be due to steady shocks in the jet and the only obvious explanation is that the source is varying.

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