Abstract
The ejected material by a SN explosion interacts with the surrounding environment, giving rise to a new astrophysical object known as SNR (for a review of this matter, I refer the reader to (Reynolds 2008) and to Appendix A for more information on the first evolutionary phase).
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Notes
- 1.
The Rayleigh-Taylor instabilities are those produced between two fluids of different densities in which the lighter pushes the heavier fluid.
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Fernández Barral, A. (2018). Introduction to Pulsar Wind Nebulae. In: Extreme Particle Acceleration in Microquasar Jets and Pulsar Wind Nebulae with the MAGIC Telescopes. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-97538-2_7
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