Fig. 8.

Frequency of various stellar masses obtained from the initial mass function, ξ = ξ0Mα, normalised to give a total stellar mass of Mtotal = 4 × 1011 M⊙, α = −0.3 for 0.01 < M⊙ < 0.08, α = −1.3 for 0.08 < M⊙ < 0.5, and α = −2.35 for M⊙ > 0.5 (Salpeter 1955; Kroupa 2001). The curve (right-hand scale) shows the approximate ionising photon rate per star.
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