Fig. 13.
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Spectral evolution in the optical for the 2D b = 0.16 model and for viewing angles of 0deg (top), 90deg (middle), and 180deg (bottom). The spectra change rapidly with wavelength at earlier times and lines become narrower with time. The spectral lines at 0deg and 180deg are blueshifted and redshifted, respectively (most evident at later times).
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