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Fig. 2

Fig. 2 Refer to the following caption and surrounding text.

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Evolution of selected CSM magnetic field components for the last 500 kyr pre-SN. The blue, orange and red shading denote the MS, RSG and WR phases respectively. (a) Time evolution of rt, the radius where Br/Bϕ = 1 close to the equatorial plane. (b) Time evolution of rt/R. (c) Time evolution of Bϕ/B, where Bϕ is calculated at a distance of 1 pc from the star, for our model (blue) and with values of Zirakashvili & Ptuskin (2018) (orange). Note while R is time dependent, B is assumed to be fixed.

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