Non-linear thermal instability of optical thin molecular structures

Details Non-linear thermal instability of optical thin molecular structures Non-linear thermal instability of optical thin molecular structures

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..255p&link_type=abstract

In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 255-257 (SEE N94-22624 05-75)

Physics

Plasma Physics

Interstellar Matter, Magnetohydrodynamic Stability, Molecular Structure, Thermal Stability, Magnetohydrodynamics, Molecular Clouds, Molecular Gases, Plasma Temperature

Scientific paper

The thermal stability of interstellar molecular structures in pressure equilibrium is examined. The numerical solution for steady structures is found, and the analytical study of the nonlinear stability of the trivial solution is performed. It is determined how the molecular gas is perturbed in order to develop supercritical stability, subcritical instability, superexponential instability, or asymptotic stability. Physical processes were included to understand the effect of the processes under consideration and as a guide in more complex models.

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