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. 13.

Impact of variations in magnetar power on the optical luminosity of the he8p00 model at 300 d after explosion. The magnetar power covers from 10³⁹ up to 6.0 × 10⁴¹ erg s⁻¹. Line identifications are provided at the bottom. [See Section 9 for discussion.]

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