Kinetic temperature of massive star-forming molecular clumps measured with formaldehyde - IV. The ALMA view of N113 and N159W in the LMC

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Fig. 2

Spectra toward H₂CO clumps in N113 (left panels) and N159W (right panels; see Table 2 and, for the numbering, the left panels of Figs. 3 and 4) taken from the strongest pixel obtained with ALMA. The pixel size is 0.′′ 2 × 0.′′2. Black: para-H₂CO 3₀₃–2₀₂, red: para-H₂CO 3₂₂–2₂₁, and blue: para-H₂CO 3₂₁–2₂₀. The spectra are not smoothed, i.e., the channel widths are those given in Table 1.

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