An asymmetrical model for high-energy radiation of Cassiopeia A. Issue 2 (5th May 2022)

• Record Type: Journal Article
• Authors: Zhan, Shihong; Wang, Wei; Mou, Guobin; Li, Zhuo
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 513:Issue 2(2022)
• Page Start: 2471
• Page End: 2477
• Publication Date: 2022-05-05
• Subjects: radiation mechanisms: non-thermal -- cosmic rays -- ISM: individual objects: Cassiopeia A -- ISM: supernova remnants; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac970
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: The supernova remnant Cassiopeia A (Cas A) shows strong radiation from radio to gamma-ray bands. The mechanism of gamma-ray radiation in Cas A and its possible contribution to PeV cosmic rays are still under debate. The X-ray imaging reveals an asymmetric profile of Cas A, suggesting the existence of a jet-like structure. In this paper, we propose an asymmetrical model for Cas A, consisting of a fast moving jet-like structure and a slowly expanding isotropic shell. This model can account for the multiwavelength spectra of Cas A, especially for the power-law hard X-ray spectrum from ∼60 to 220 keV. The GeV to TeV emission from Cas A should be contributed by both hadronic and leptonic processes. Moreover, the jet-like structure may produce a gamma-ray flux of $\sim 10^{-13}\rm erg\, cm^{-2}\, s^{-1}$ at ∼100 TeV, to be examined by the Large High Altitude Air Shower Observatory (LHAASO) and the Cherenkov Telescope Array (CTA).