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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Radio/IR relation!<br />
• Global (de Jong et al. 85, Condon 92,<br />
Bell 03….)<br />
• & local (Murphy et al. 06, Tabatabei<br />
et al. 07…)<br />
• L<strong>in</strong>ear relation<br />
Infrared Emission, ISM and Star Formation!<br />
Dumas Gaelle, February 24 th 2010!<br />
q = log(FIR/20cm) quantitative<br />
measure <strong>of</strong> <strong>the</strong> radio/IR correlation<br />
From Bell 03<br />
<strong>M51</strong>