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Fig. 2

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Density, temperature, and velocity profiles of a PION simulation with a single star model of Z = 0.004, υini = 0 km s−1, and log10(M/M) = 1.5 in a uniform medium of n = 100 cm−3 at 5 Myr (top), at the end of the stellar lifetime (middle), and 5 Myr after the subsequent SN (bottom). Dashed lines indicate negative velocities. The circled numbers at the top indicate the five different regions found in the density profile due to pre-SN feedback.

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