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Park, Jaegeun; Kim, Chanho; Woo, Jooyun; An, Hongjun; Mori, Kaya; Reynolds, Stephen P.; Safi-Harb, Samar
The Astrophysical journal, 03/2023, Letnik: 945, Številka: 1Journal Article
Abstract We report on broadband X-ray properties of the Rabbit pulsar wind nebula (PWN) associated with the pulsar PSR J1418−6058 using archival Chandra and XMM-Newton data, as well as a new NuSTAR observation. NuSTAR data above 10 keV allowed us to detect the 110 ms spin period of the pulsar, characterize its hard X-ray pulse profile, and resolve hard X-ray emission from the PWN after removing contamination from the pulsar and other overlapping point sources. The extended PWN was detected up to ∼20 keV and is described well by a power-law model with a photon index Γ ≈ 2. The PWN shape does not vary significantly with energy, and its X-ray spectrum shows no clear evidence of softening away from the pulsar. We modeled the spatial profile of X-ray spectra and broadband spectral energy distribution in the radio to TeV band to infer the physical properties of the PWN. We found that a model with low magnetic field strength ( B ∼ 10 μ G) and efficient diffusion ( D ∼ 10 27 cm 2 s −1 ) fits the PWN data well. The extended hard X-ray and TeV emission, associated respectively with synchrotron radiation and inverse Compton scattering by relativistic electrons, suggest that particles are accelerated to very high energies (≳500 TeV), indicating that the Rabbit PWN is a Galactic PeVatron candidate.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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