Disentangling emission from star-forming regions in the Magellanic Clouds: Linking [O iii]λ88 µm and 24 µm

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Volume 666 (October 2022)

A&A, 666 (2022) A112

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Table 5

Solutions for constant pressure models that reproduce the full global data set of all regions together as well as the individual regions.

	Best model log(U), log(n₀)	Other agreeing models log(U), log(n₀)
Global sample	−3,2.5	−2, [1.5,2]
30 Doradus		−3, [2,2.5]
	−3,2.5	−3, [1.5,2]
		−2, [1.5,2]
N11B	−3, [2,2.5]	−
N11C	−3,2	−3,2.5
N11I	−3,2	−3,2.5
N44	−2,1.5	−2,2
		−3, [2.5, 3]
N158	−3,2.5	−2,1.5
N159	−3,2.5	−2, [1.5,2]
N160	−3,2.5	−2, [1.5,2]
N180	−3, [2,2.5]	−2,1.5
N66	−3,2	−

Notes. As the observations trace a wide range in parameter space, other models of our grid can be consistent with each region (although less than our best model), or with a subpart of the region. Those models are indicated in the third column of the table.

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