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A Quarter Century of Guitar Nebula/Filament Evolution

Abstract:
We have collected a new deep Chandra X-Ray Observatory exposure of PSR B2224+65 and the "Guitar Nebula," mapping the complex X-ray structure. This is accompanied by a new Hubble Space Telescope (HST) Hα image of the head of the Guitar. Comparing the HST and Chandra structures in four epochs over 25 yr, we constrain the evolution of the TeV particles that light up the filament. Cross-field diffusion appears to be enhanced, likely by the injected particles, behind the filament's sharp leading edge, explaining the filament width and its evolving surface brightness profile...
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4357/ac9794

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Role:
Author
ORCID:
0000-0001-5282-0404
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Role:
Author
ORCID:
0000-0001-6711-3286
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Role:
Author
ORCID:
0000-0002-6447-4251
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Role:
Author
ORCID:
0000-0002-7481-5259
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0003-2317-9747


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Funder identifier:
10.13039/100000104
Grant:
G08-19050A


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal More from this journal
Volume:
939
Issue:
2
Pages:
70-70
Publication date:
2022-11-08
DOI:
EISSN:
1538-4357
ISSN:
0004-637X


Language:
English
Keywords:
Pubs id:
1310872
Local pid:
pubs:1310872
Source identifiers:
W4308579298
Deposit date:
2026-04-30
ARK identifier:
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