The physics of the star formation process in M51

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Infrared Emission, ISM and Star Formation!

Dumas Gaelle, February 24 th 2010!

Radio/IR relation!

Outer disk Inner region Non linear : 24µm α (20cm) 1.5

Non linear : 24µm α (20cm) 0.5

Power law fit: 24µm = b (20cm) a

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• Schmidt law Infrared Emission, ISM and Star Formation! Dumas Gaelle, February 24 th 2010! • Niklas & Beck, 1997 • Beck et al., 1996 Non linearity in interarm!

Infrared Emission, ISM and Star Formation! Dumas Gaelle, February 24 th 2010! Radio/IR relation! Outer disk Inner region Non linear : 24µm α (20cm) 1.5 Non linear : 24µm α (20cm) 0.5 Power law fit: 24µm = b (20cm) a

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The physics of the star formation process in M51

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