Magneto-archeology of white dwarfs - Revisiting the fossil field scenario with observational constraints during the red giant branch

Open Access

Fig. E.2.

2D slice of the magnetic field of Scenario C at the start of the WD cooling sequence. Left: Local magnetic field strength $\sqrt{B \cdot B}$ $Mathematical equation: $ \sqrt{\boldsymbol{B}\cdot\boldsymbol{B}} $$ throughout the full WD. The yellow region shows where most of the magnetic field strength is located. Right: Corresponding field lines to the same magnetic field shown on the left.

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