Multi-GeV lightcurves: possible hints for the emission mechanism

DOI オープンアクセス

説明

Although the Fermi observatory has reported delayed onsets of GeV emissions, the photon statistics are not sufficient to distinguish the emission mechanisms. Future multi-GeV observations such as CTA may give us precise lightcurves that can be compared with lower energy bands. In this paper we show our time-dependent simulations for leptonic and hadronic models. Our results suggest that the multi-GeV lightcurves are powerful tool to probe the GeV emission mechanisms.

収録刊行物

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