All Figures

	Figure 1: The 3.6 cm radio map of M 33 ( left panel) observed with the 100-m radio telescope in Effelsberg, and the combined 20 cm radio map ( right panel) from the VLA and Effelsberg observations. The half power beam widths ( HPBWs) of and , respectively, are shown in the lower left corners.
Open with DEXTER


In the text

	Figure 2: Top: the Spitzer MIPS images of M 33 at 24 m ( left panel) and 70 m ( right panel). Bottom: the Spitzer MIPS image at 160 m ( left panel) and the H map ( right panel) from KPNO Hoopes & Walterbos (2000). The resolutions are given in Table 1.
Open with DEXTER


In the text

Figure 3: MIPS maps of M 33 at resolution ( first column) and their wavelet decompositions for 4 different scales: ( second column), ( third column), ( forth column), and ( fifth column). At the distance of 840 kpc, is equivalent to 4 pc. The maps at 24, 70, and 160 m are shown from top to bottom. Before the decomposition, huge HII regions like NGC 604 were subtracted from the original images (Sect. 4). Maps are shown in RA-Dec coordinate system and centered at the center of the galaxy. The field size is    .

Open with DEXTER


In the text

	Figure 4: The wavelet spectra of the 24 and 70 m images before (or.) and after (s.s.) subtraction of the same sources from the two images at resolution. The data points correspond to the scales 34, 50, 73, 107, 155, 226, 329, 479, 697, . The spectra are shown in arbitrary units.
Open with DEXTER


In the text

	Figure 5: The wavelet spectra of the 20 cm radio and IR images at resolution before ( left) and after ( right) subtraction of the same sources. For comparison, the wavelet spectrum of the H emission is also plotted. The data points correspond to the scales 112, 143, 183, 234, 299, 383, 490, 626, 800, . The spectra are shown in arbitrary units.
Open with DEXTER


In the text

	Figure 6: The wavelet spectra of the 3.6 cm radio and IR images at resolution before ( left) and after ( right) subtraction of the same sources. For comparison, the spectrum of the H emission is also plotted. The data points correspond to the scales 210, 250, 298, 356, 424, 505, 602, 718, 856, . The spectra are shown in arbitrary units.
Open with DEXTER


In the text

	Figure 7: The cross-correlation between 24 and 70 m ( top), 24 and 160 m ( middle), and 70 and 160 m ( bottom) images at resolution before (or.) and after (s.s.) source subtraction.
Open with DEXTER


In the text

	Figure 8: The cross-correlation between 3.6 cm radio and IR before and after subtraction of the same sources at resolution.
Open with DEXTER


In the text

	Figure 9: The correlation of the 20 cm radio and IR before and after subtraction of the same sources at resolution (please note that this figure starts from 100 and not 200 ).
Open with DEXTER


In the text

	Figure 10: The correlation of H with IR ( top) at and with 3.6 and 20 cm radio ( bottom) at resolution. The maps include allHII regions.
Open with DEXTER


In the text