Guitar nebula: Extreme accelerator in extreme environment — E8 Intelligence Research

Guitar nebula is a prime example of a class of bow-shock pulsar wind nebulae (PWNe), powered by a wind of a supersonically moving neutron star. Bow-shock PWNe can probe particle acceleration processes in relativistic pulsar winds, as well as the structure of the interstellar medium (ISM). We demonstrate that Guitar is an exceptional object in a number of ways. First, particles escaping the PWN and forming the X-ray "kinetic jet" need to be accelerated to the energies corresponding to the maximal electric potential of the neutron star ηacc≳3/4 : it is another example of the class of extreme accelerators. Second, exceptionally bright Hα emission requires that the central pulsar PSR J2225+6535 passes through a dense, low ionization ISM region. Bright X-ray emission of the "kinetic jet" then also requires excep Author: Andrew Stewart Caldin, Independent Researcher, UK. Part of the E8 Intelligence Research series. Platform: e8intelligence.com

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-06
DOI
https://doi.org/10.5281/zenodo.23998410
Primary Topic
Astrophysics and Cosmic Phenomena
Type
preprint
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Guitar nebula: Extreme accelerator in extreme environment — E8 Intelligence Research

Andrew Stewart Caldin
Zenodo (CERN European Organization for Nuclear Research)
Astrophysics and Cosmic Phenomena
preprint

Guitar nebula: Extreme accelerator in extreme environment — E8 Intelligence Research

Andrew Stewart Caldin
preprint en

Abstract

Guitar nebula is a prime example of a class of bow-shock pulsar wind nebulae (PWNe), powered by a wind of a supersonically moving neutron star. Bow-shock PWNe can probe particle acceleration processes in relativistic pulsar winds, as well as the structure of the interstellar medium (ISM). We demonstrate that Guitar is an exceptional object in a number of ways. First, particles escaping the PWN and forming the X-ray "kinetic jet" need to be accelerated to the energies corresponding to the maximal electric potential of the neutron star ηacc≳3/4 : it is another example of the class of extreme accelerators. Second, exceptionally bright Hα emission requires that the central pulsar PSR J2225+6535 passes through a dense, low ionization ISM region. Bright X-ray emission of the "kinetic jet" then also requires excep Author: Andrew Stewart Caldin, Independent Researcher, UK. Part of the E8 Intelligence Research series. Platform: e8intelligence.com

Zenodo (CERN European Organization for Nuclear Research)
Astrophysics and Cosmic Phenomena
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