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Fig. 3

image

Illustration of the ejecta regions (in velocity space) at the origin of the optical flux for model DDC15 with Mst = 0.18 M at 200 d. The top panel shows a gray linear scale of the (emergent) luminosity δLλ,V while the bottom panel shows the contributions (ordinate in logarithmic space) for the full ejecta and those fromthe stripped material (blue) or the metal-rich ejecta (red). As is evident from these plots, the predominant emerging feature due to stripped material of the companion star at optical wavelengths is Hα.

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