Fig. 7
Top: model variations of the nebular continuum radiation in SY Mus (Eq. (3)) at ten wavelengths (solid lines). They are compared with the nebular fluxes at ϕ = 0.62 from the model SED (circles with errorbars). Bottom: model SED of SY Mus at ϕ = 0.62. Circles at the nebular component correspond to those plotted at the top panel.
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