Hα and [N II] spectral lines from the simulation M5V20E, with Ṁ = 2 × 10-5 M⊙ yr-1, v∞ = 20 km s-1, and Fγ = 2.78 × 1010 cm-2 s-1, after 0.1 Myr of evolution. The solid lines show the simulation, and the dotted lines with points show the observations to the ESE of W26. The panels show a) line brightness; b) line ratio [N II]/Hα; and c) radial velocity of the peak emission, all as a function of distance from the star.
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