Proper motion, spectra, and timing of PSR J1813–1749 using Chandra and NICER

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 Chandra datasets that are separated by more than ten years and recent NICER d...

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Pubblicato in:Mon Not R Astron Soc
Autori principali: Ho, Wynn C. G., Guillot, Sebastien, Parkinson, P.M. Saz, Limyansky, B., Ng, C.-Y., Bejger, Michał, Espinoza, Cristóbal M., Haskell, B., Jaisawal, Gaurava K., Malacaria, C.
Natura: Artigo
Lingua:Inglês
Pubblicazione: 2020
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Article
Accesso online:https://ncbi.nlm.nih.gov/pmc/articles/PMC7668304/
https://ncbi.nlm.nih.gov/pubmed/33204043
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnras/staa2653
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