Fig. 6
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Para-H2CO (303 –202) with integrated intensity contours (same as Fig. 1) overlaid on Hα (left panels; Smith & MCELS Team 1998), Spitzer 8.0 μm (middle panels; Meixner et al. 2006), and 1.3 mm continuum (right panels; observed with ALMA Band 6; Fukui et al. 2015; Sewiło et al. 2018) images of N113 (top panels) and N159W (bottom panels). Stars and triangles show the locations of the YSOs (or YSO candidates) and H2O masers (Chen et al. 2010; Ellingsen et al. 2010; Carlson et al. 2012), respectively.
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