Research Article

Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions

Figure 15

The IMF power-law slope as a function of the PDMF power-law slope for the case of episodic star formation. In each panel the lowest line is Δ 𝑡 = 1 0 8 y r s and the highest line is Δ 𝑡 = 1 0 6 y r s .
174105.fig.0015a
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174105.fig.0015b
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174105.fig.0015c
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