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. Khangulyan, 8] proposent une interaction entre les photons infrarouge du disque circumstellaire avec des électrons du vent du pulsar, cette interaction augmente après que le pulsar ait traversé une deuxième fois le disque circumstellaire, Bien que trois éruptions aient été maintenant observées, l'origine de ces événements n'est toujours pas éclaircie, 2012.

, 2014 (orange) et 2017 (en vert). L'intervalle choisi sur les courbes de lumière est de 7 jours et l'origine des temps est choisie au moment du passage du périastre. Le profil est clairement différent par rapport aux courbes de lumière obtenues dans le domaine du TeV (voir figures 8, FIGURE 8.8-Courbes de lumière pour E > 100 MeV mesurées par le satellite Fermi-LAT

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