Temporal evolution of magnetic molecular shocks II. Analytics of the steady state and semi-analytical construction of intermediate ages
P. Lesaffre, J.-P. Chi\`eze, S. Cabrit, G. Pineau des For\^ets

TL;DR
This paper develops analytical models for steady-state molecular shocks, verifies their applicability to intermediate ages in time-dependent simulations, and introduces a semi-analytical method to construct low-velocity shock states efficiently.
Contribution
It derives new relationships for steady-state shock structures and introduces a semi-analytical construction method for intermediate shock ages using steady-state codes.
Findings
Most stable shocks are in a quasi-steady state at all times.
The semi-analytical method accurately predicts steady CJ-type shocks.
Steady-state equations are valid for intermediate ages in time-dependent shocks.
Abstract
In the first paper of this series (Paper I) we computed time dependent simulations of multifluid shocks with chemistry and a transverse magnetic field frozen in the ions, using an adaptive moving grid. In this paper, we present new analytical results on steady-state molecular shocks. Relationships between density and pressure in the neutral fluid are derived for the cold magnetic precursor, hot magnetic precursor, adiabatic shock front, and the following cooling layer. The compression ratio and temperature behind a fully dissociative adiabatic shock is also derived. To prove that these results may even hold for intermediate ages, we design a test to locally characterise the validity of the steady state equations in a time-dependent shock simulation. Applying this tool to the results of Paper I, we show that most of these shocks (all the stable ones) are indeed in a quasi-steady state at…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Astrophysics and Star Formation Studies · Astro and Planetary Science
