Fig. 5.
Polarisation (bottom panel) and polarisation angle (top panel) observed towards the Fried Egg Nebula. The black dots represent the broadband values, computed in steps of 10 nm, or 100 Å, from the spectropolarimetric data. The red triangles represent the Lebertre et al. (1989) data. The dashed line is the best-fit Serkowki law for interstellar polarisation.
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