Suppression of X-rays from radiative shocks by their thin-shell instability
Publication date: 25 January 2014
Authors: N. D. Kee, et al.
Journal: Monthly Notices of the Royal Astronomical Society
Copyright: The Royal Astronomical Society
We examine X-rays from radiatively cooled shocks, focusing on how their thin-shell instability reduces X-ray emission. For 2D simulations of collision between equal expanding winds, we carry out a parameter study of such instability as a function of the ratio of radiative versus adiabatic-expansion cooling lengths. In the adiabatic regime, the extended cooling layer suppresses instability, leading to planar shock compression with X-ray luminosity that follows closely the expected ( LX∼M_dot2 ) quadratic scaling with mass-loss rate M_dot. In the strongly radiative limit, the X-ray emission now follows an expected linear scaling with mass-loss (LX∼M_dot), but the instability deforms the shock compression into extended shear layers with oblique shocks along fingers of cooled, dense material. The spatial dispersion of shock thermalization limits strong X-ray emission to the tips and troughs of the fingers, and so reduces the X-ray emission (here by about a factor 1/50) below what is expected from analytic radiative-shock models without unstable structure. Between these two limits, X-ray emission can switch between a high-state associated with extended shock compression, and a low-state characterized by extensive shear. Further study is needed to clarify the origin of this ‘shear mixing reduction factor’ in X-ray emission, and its dependence on parameters like the shock Mach number.Link to publication