A Comprehensive Study of the Spectral Variation and the Brightness Profile of Young Pulsar Wind Nebulae
arXiv:2201.09403 · doi:10.3847/1538-4357/ac4d2d
Abstract
We present a systematic study of particle transport by diffusion in young pulsar wind nebulae (PWNe). We selected nine bright sources that are well resolved with the Chandra X-ray Observatory. We analyzed archival data to obtain their radial profiles of photon index () and surface brightness () in a consistent way. These profiles were then fit with a pure diffusion model that was tested on Crab, 3C 58 and G21.50.9 before. In addition to the spectral softening due to the diffusion, we calculated the synchrotron power and built up the theoretical surface brightness profile. For each source, we performed separate fits to the and the profiles. We found these two profiles of most PWNe are similar, except for Crab and Vela. Both profiles can be well described by our model, suggesting that diffusion dominates the particle transport in most sampled PWNe. The discrepancy of parameters between the profile and profiles is relatively large for 3C 58 and G54.1+0.3. This difference could be attributed to the elongated shape, reflecting boundary, and the non-uniform magnetic field. Finally, we found no significant correlations between diffusion parameters and physical parameters of PWN and pulsar.
15 pages, 6 figures, accepted for publication in ApJ
References in corpus (6)
- Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
- Magnetar-like Emission from the Young Pulsar in Kes 75
- Fitting Pulsar Wind Tori. II. Error Analysis and Applications
- Deep Chandra Observation of the Pulsar Wind Nebula Powered by the Pulsar J1846-0258 in the Supernova Remnant Kes 75
- A Shell of Thermal X-ray Emission Associated with the Young Crab-like Remnant 3C58
- Revealing Hidden Variability in PWNe With Spectral Index Maps
Cited by in corpus (5)
- Revisiting the Chandra Observation on the Region of PSR J1809-1917: Indication of an X-ray Halo and Implication for the Origin of HESS J1809-193
- Spectral Break of Energetic Pulsar Wind Nebulae Detected with Wideband X-ray Observations
- Pulsar Wind Nebulae
- Spatial Variations and Breaks in the Optical-NIR spectra of the Pulsar and PWN in SNR 0540-69.3
- Spatio-spectral-temporal Modelling of Two Young Pulsar Wind Nebulae