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- [2105. 09155] Probing the hadronic nature of the gamma-ray emission . . .
In this paper, we analyze more than 11 years of Fermi-LAT data from the direction of Westerlund 2, one of the most massive and best-studied star-forming regions in our Galaxy
- Probing the hadronic nature of the gamma-ray emission associated with . . .
This identification provides new clues about the origin of the HESS J1023-575 gamma-ray emission, favouring a hadronic origin of the emission, powered by Westerlund 2, rather than a leptonic origin related to either the pulsar wind nebula associated with PSR J1023–5746 or the cluster itself
- Probing the hadronic nature of the gamma-ray emission associated with . . .
PDF | On Jul 15, 2021, Emma Maria de Ona Wilhelmi and others published Probing the hadronic nature of the gamma-ray emission associated with Westerlund 2 | Find, read and cite all the
- Probing the hadronic nature of the gamma-ray emission . . . - NASA ADS
This identification provides new clues about the origin of the HESS J1023-575 gamma-ray emission, favouring a hadronic origin of the emission, powered by Westerlund 2, rather than a leptonic origin related to either the pulsar wind nebula associated with PSR J1023-5746 or the cluster itself
- ONLINE ICRC ICRC 2021
The combined results provide new hints on the origin of the GeV and TeV emission and its connection with Westerlund 2
- Probing the hadronic nature of the gamma-ray emission associated with . . .
We analyze more than 11 years of Fermi-LAT data from the direction of Westerlund 2, one of the most massive and best-studied star-forming regions in our Galaxy
- Probing the hadronic nature of the gamma-ray emission associated with . . .
This identification provides new clues about the origin of the HESSJ1023-575 gamma-ray emission, favouring a hadronic origin of the emission, powered by Westerlund 2, rather than a leptonic origin related to either the pulsar wind nebula associated with PSRJ1023–5746 or the cluster itself
- Probing the hadronic nature of the gamma-ray emission associated
S J1023-575, through its morphological and spec-tral properties This identication provides new clues about the origin of the HESS J1023-575 gamma-ray emission, favouring a hadronic origin of the emission, powered by Westerlund 2, rather than a leptonic origin related to either the pulsar
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