Fig. B.2
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Images of the thermal reemission radiation of the dust shell outburst model after 1000, 2000 and 3000 s at a wavelength of 10 µm as described in Sect. B (temporal step width: 1000 s). The flux is normalized with respect to the maximum flux of the image after 1 000 s. The white dotted lines indicate the maximum radius of the parabola depicted in Fig. B.1.
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