Observations of the γ-ray pulsar J1932+1916 in X-rays

We present the analysis of the archival Suzaku and Swift X-ray observations of the young gamma -ray pulsar J1932+1916 field. The data revealed a point-like object at the gamma -ray position of the pulsar and diffuse X-ray emission around it. Spectra of the point-like source and diffuse emission are...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2017-04, Vol.466 (2), p.1757-1763
Main Authors: Karpova, A., Shternin, P., Zyuzin, D., Danilenko, A., Shibanov, Yu
Format: Article
Language:English
Subjects:
Emission
Mathematical models
Nebulae
Pulsars
Spectral emissivity
Stellar winds
Supernova remnants
X rays
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