Nonlinear Development and Observational Consequences of Wardle C-Shock Instabilities

Details Nonlinear Development and Observational Consequences of Wardle C-Shock Instabilities Nonlinear Development and Observational Consequences of Wardle C-Shock Instabilities

1997-03-26

arxiv.org/abs/astro-ph/9703172v1

Astronomy and Astrophysics

Astrophysics

24 pages, 18 figures, uses aaspp4.sty, submitted to ApJ, 26 March 1997 Larger figures are jpegs; original postscript is availa

Scientific paper

10.1086/304981

We compute the nonlinear development of the instabilities in C-shocks first described by Wardle, using a version of the ZEUS code modified to include a semi-implicit treatment of ambipolar diffusion. We find that, in three dimensions, thin sheets parallel to the shock velocity and perpendicular to the magnetic field lines form. High resolution, two-dimensional models show that the sheets are confined by the Brandenburg & Zweibel ambipolar diffusion singularity, forcing them to numerically unresolvable thinness. Hot and cold regions form around these filaments, disrupting the uniform temperature structure characteristic of a steady-state C-shock. This filamentary region steadily grows as the shock progresses. We compare steady-state to unstable C-shocks, showing excitation diagrams, line ratios, and line profiles for molecular hydrogen lines visible in the K-band, with the Infrared Space Observatory, and with NICMOS on the Hubble Space Telescope.

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