Table 1: Images of M 33 used in this study.
Wavelength Resolution Telescope
20 cm $51\hbox {$^{\prime \prime }$ }$ VLA 1
20 cm $540\hbox{$^{\prime\prime}$ }$ Effelsberg 2
3.6 cm $84\hbox {$^{\prime \prime }$ }$ Effelsberg1
160 $\mu $m $40\hbox {$^{\prime \prime }$ }$ Spitzer3
70 $\mu $m $18\hbox {$^{\prime \prime }$ }$ Spitzer3
24 $\mu $m $6\hbox{$^{\prime\prime}$ }$ Spitzer3
6570Å (H$\alpha $) $2\hbox{$^{\prime\prime}$ }$ (pixel size) KPNO4
1 Tabatabaei et al. (in prep.).
2 Fletcher (2001).
3 Hinz et al. (2004) and this paper.
4 Hoopes & Walterbos (2000).


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