Observable and ionizing properties of star-forming galaxies with very massive stars and different initial mass functions

Open Access

Fig. 2.

Predicted temporal evolution of the ionizing photon production, Q_H, of different models, for instantaneous bursts and constant SFR. Burst models are normalized to 10⁶ M_⊙, models for constant SFR to SFR = 1 M_⊙ yr⁻¹.

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