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. 9.

Influence of clumping on ejecta properties for model he6p00 at 2200 d and influenced by a magnetar power of 10³⁹ erg s⁻¹. The adopted clumping is uniform and corresponds to a volume filling factor from 100% (smooth ejecta) down to 5%.

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