Fig. 5
Methanol maser flux vs. distance of the associated clump for all masers found by Pandian et al. (2007) (red triangles) and our newly detected methanol masers (black “+” signs). The median value of the integrated flux density of our own masers is ≃0.03 Jy km s-1, while the median value for the AMGPS masers is ≃1.6 Jy km s-1.
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