The long-term influence of a magnetar power in stripped-envelope supernovae - Radiative-transfer modeling of He-star explosions from 1 to 10 years

Open Access

Fig. B.5.

Same as Fig. 4 but now for model he3p30 at 2200 d, influenced by a power of 10³⁹ erg s⁻¹. Volume-integrated cooling powers are given for this model in Table 6. [See Section 5.3 for discussion.]

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