The physics of the star formation process in M51
The physics of the star formation process in M51
The physics of the star formation process in M51
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Infrared Emission, ISM and Star Formation!<br />
Dumas Gaelle, February 24 th 2010!<br />
• NT radio: synchrotron<br />
emission,<br />
• <strong>The</strong>rmal radio<br />
• IR: heated dust<br />
Radio/IR relation!<br />
arms Interarm<br />
Power law fit: 24µm = b (20cm) a
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