Molecular clouds under the influence of massive stars in the Galactic Hii region G353.2+0.9

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Table 3

Gas masses derived from dust emission.

Component	Mass	Associated molecular clumps
	(M_⊙)

1	370	C1
2	180	C2
3	210	H, F
4	340	E
5¹	360	D, A, B
Total²	2100

Notes. The gas-to-dust ratio was assumed to be γ = 100. The total mass is computed by integrating the total 870 μm flux.

⁽¹⁾

Not a Gaussian fit, but a region that comprises all the emission at the corresponding location.

⁽²⁾

computed integrating the whole 870 μ flux.

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