Proper motion, spectra, and timing of PSR J1813-1749 using
HESS J1813–178 – ISM: supernova remnants – pulsars: general – pulsars: individual: CXOU J181335.16–174957.4
ISM: individual: G12.82–0.02
PSR J1813–1749–X-rays: stars
Journal
Monthly notices of the Royal Astronomical Society
ISSN: 0035-8711
Titre abrégé: Mon Not R Astron Soc
Pays: England
ID NLM: 100954591
Informations de publication
Date de publication:
Nov 2020
Nov 2020
Historique:
entrez:
18
11
2020
pubmed:
19
11
2020
medline:
19
11
2020
Statut:
ppublish
Résumé
PSR J1813-1749 is one of the most energetic rotation-powered pulsars known, producing a pulsar wind nebula (PWN) and gamma-ray and TeV emission, but whose spin period is only measurable in X-ray. We present analysis of two
Identifiants
pubmed: 33204043
doi: 10.1093/mnras/staa2653
pmc: PMC7668304
mid: NIHMS1640442
doi:
Types de publication
Journal Article
Langues
eng
Pagination
4396-4403Subventions
Organisme : Intramural NASA
ID : 80NSSC19K1444
Pays : United States
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