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From the following article:

Clustered star formation as a natural explanation for the Halpha cut-off in disk galaxies

Jan Pflamm-Altenburg & Pavel Kroupa

Nature 455, 641-643(2 October 2008)

doi:10.1038/nature07266

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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

Halpha luminosity surface density (SigmaHalpha) versus total gas surface density (Sigmagas).

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Figure 2 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 2

Star-formation-rate surface density (SigmaSFR) versus galactocentric radius (r).

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