Sentence examples for by the reverse shock from inspiring English sources

The emission from the ejecta heated by the reverse shock dominates that from the ISM heated by the blast wave.

The dotted lines are the size distribution expected after the grain destruction by the reverse shock in the supernova remnant by Nozawa et al. (2007).

In addition, we adopt the size distribution expected by Nozawa et al. (2007), who explored the effect of the dust destruction by the reverse shock in the SN remnant, as the N07 model.

In contrast, the heating rate with the size distribution of the grains processed by the reverse shock in the supernova remnant is a factor of ∼3 smaller than that with the MRN model.

The X-ray spectral features of N49 suggest that the post-shock regions in the east might have been reheated by the reverse shock off the dense clouds, while the blast wave shock front has decelerated as it propagates into the clouds.

We propose that the expansion of the small-scale bright ring features in the optical, X-ray, and radio do not represent the expansion of the reverse shock, but rather represent a brightness-weighted average of ejecta passing through and being decelerated by the reverse shock.

Moreover, the dust production by SNe is further complex because the reverse shock moving in the ejecta of an SN may destroy the dust produced in the ejecta (Bianchi and Schneider, 2007; Nozawa et al., 2007; Nath et al., 2008; Silvia et al., 2010).

The motion of the reverse shock is represented by the motion of the angle-averaged emissivity profile of the radio bright ring.

The strongly off-centered position of the pulsar with respect to its pulsar wind nebula is naturally explained by the result of the interaction of the reverse shock with the pulsar wind nebula, as the simulation bears out.

A second shock wave, the reverse shock, may propagate back into the ejected matter.

The reverse shocks were more oblique (average θnBo = 52o), but they extended to all angles.