Categories Cosmic Ray Indirect Supernova remnant G106.3+2.7: a likely proton PeVatron

Supernova remnant G106.3+2.7: a likely proton PeVatron

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  • uploaded June 26, 2021

Discussion timeslot (ZOOM-Meeting): 20. July 2021 - 12:00
ZOOM-Meeting URL: https://desy.zoom.us/j/98542982538
ZOOM-Meeting ID: 98542982538
ZOOM-Meeting Passcode: ICRC2021
Corresponding Session: https://icrc2021-venue.desy.de/channel/46-Supernova-Remnants-GAD-GAI-CRD/76
Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-04/5

Abstract:
'We analyze the data of Chandra and XMM-Newton in the region of SNR G106.3+2.7 and find the spectrum is dominated by non-thermal X-ray radiation of electrons. The X-ray surface brightness profile of the SNR indicates that the X-ray-emitting electrons in the tail region of the SNR is accelerated by the SNR shock, implying the SNR is an efficient particle accelerator. Based on the multiwavelength data of the SNR, we suggest that the tail region of the SNR is likely a proton PeVatron.'

Authors: Ruo-Yu Liu | Chong Ge | Shu Niu | Yang Chen | Xiang-Yu Wang
Indico-ID: 91
Proceeding URL: https://pos.sissa.it/395/287

Tags:
Categories: Cosmic Ray Indirect, Scientific Contributions
Presenter: Ruo-Yu Liu

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