MHD lensing in inhomogeneous ISM for qualitative understanding of the morphology of supernova remnants

TL;DR

This paper explores how inhomogeneous interstellar medium affects the morphology of supernova remnants by modeling MHD wave lensing, revealing diverse structures like filaments and arcs that resemble observed remnants.

Contribution

It introduces a qualitative model of MHD wave lensing in inhomogeneous ISM to explain complex supernova remnant morphologies.

Findings

High Alfvén velocity clouds act as concave lenses diverging waves.

Low Alfvén velocity clouds act as convex lenses converging waves.

Various cloud types produce diverse remnant-like structures.

Abstract

Morphological evolution of expanding shells of fast-mode magnetohydrodynamic (MHD) waves through an inhomogeneous ISM is investigated in order to qualitatively understand the complicated morphology of shell-type supernova remnants (SNR). Interstellar clouds with high Alfv\'en velocity act as concave lenses to diverge the MHD waves, while those with slow Alfv\'en velocity act as convex lenses to converge the waves to the focal points. By combination of various types of clouds and fluctuations with different Alfv\'en velocities, sizes, or wavelengths, the MHD-wave shells attain various morphological structures, exhibiting filaments, arcs, loops, holes, and focal strings, mimicking old and deformed SNRs.