Abstract
Chapter 5 describes the evolution of supernova remnants in the context of simplified description using consecutive phases: the ejecta dominated phase, the energy-conservation (Sedov-Taylor) phase, and the pressure-driven phase. In this chapter we will discuss the current observational status of our knowledge concerning young supernova remnants, supernova remnants up to 2000 yr old, which are either in the ejecta dominated, or in the Sedov-Taylor phase. However, here we are not so much concerned with actual phase the supernova remnants are in, but more with what the observed properties of the supernova remnants tells us about the supernova explosions through the composition and distribution of the supernova ejecta, and about their progenitor stars, through the imprint their wind has had on the ambient medium. An important property of the youngest supernova remnants is their ability to accelerate particles beyond 10 TeV; this aspect of young supernova remnants is discussed in Chap. 12.
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Notes
- 1.
This is a revised and extended version of a section in [1173].
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Vink, J. (2020). Young Supernova Remnants: Probing the Ejecta and the Circumstellar Medium. In: Physics and Evolution of Supernova Remnants. Astronomy and Astrophysics Library. Springer, Cham. https://doi.org/10.1007/978-3-030-55231-2_9
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