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Fig. 2.
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Time evolution of the bolometric luminosity of novae breves for different EOSs and magnetar masses. Different colors correspond to different EOSs. Solid lines show the results for a 1.4 M⊙ magnetar, while dashed lines correspond to the 2.0 M⊙ case. The magnetic field strength is considered to be B ≃ 1015 G.
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