Fig. 15
Scatter plots of the dust emissivity index β versus the Hα, CO(1 − 0), and HI emission from M 33. The y-axis presents the logarithm of the intensities in units of cm-6 pc for the Hα emission and K km s-1 for the CO(1 − 0) and HI emssions. Also shown are Pearson correlation coefficients (r), the ordinary least-squares (OLS) fits, and the bisector fits.
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