Pulsar wind nebulae - Open Access .click

Письма в Астрономический журнал: Астрономия и космическая астрофизика, 2023
Transonic (withMach numberMs 1) motion of a pulsar relative to the external medium canhelp its compact pulsar wind nebula develop a double-torus X-ray morphology. The double-torus structurecan reverberate as a whole under the dynamic pressure of the external flow. For a flow aligned with thesymmetry axis of the nebula, the response of the double-torus
A. E. Petrov, K. P. Levenfish, G. A. Ponomaryov +2 more
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Pulsars and Pulsar Wind Nebulae

2019
When heavy stars have burned all their nuclear fuel, neutron degeneracy pressure is the last force able to halt their collapse into a black hole. The sudden stop of the free-fall collapse leads to a rebound of the infalling matter triggering an outward shock that blows up the star envelope and powers a Type II supernova.
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Neutron Stars, Pulsars, and Pulsar Wind Nebulae

2020
The connection between supernovae and neutron stars goes back to the seminal publications by W. Baade and F. Zwicky in 1934, in which they coined both the term “super-nova”, suggested a connection between cosmic rays and “super-novae” and postulated that a “super-nova” event “represents the transition of an ordinary star into a neutron star”.
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pulsars
stars
nebula

supernova remnants
quantum mechanics
galaxy

pulsar wind nebula
heliosphere
solar wind