Fig. 5

Emergent intensity from the surface of ϕ Dra at various rotational phases at wavelengths of 1400 Å (left panel), 2500 Å (middle panel), and in the U-band of the ten-colour system (right panel). The intensities are displayed as −2.5log (I/I0), where I0 is a reference intensity chosen in such a way that the resulting logarithm, averaged over the entire stellar surface, is equal to zero.
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