Toward a better understanding of the mid-infrared emission in the Large Magellanic Cloud

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Table 1

Characteristics of the studied regions.

Region	Type				n_e^(★)
SSDR1	Molecular	4.8	7.3	0.50	1.52
SSDR5	Molecular	1.6	3.0	0.23	3.98

SSDR7	Diffuse	3.9	–	0.035	1.52
SSDR9	Diffuse	4.7	–	–	–

SSDR8	Ionized	1.7	–	1.7	3.98
SSDR10	Ionized	0.68	–	1.9	3.98
DEML10	Ionized	3.1	0.36	1.9	3.98
DEML34	Ionized	2.9	6.9	6.8	3.98
DEML86	Ionized	2.2	3.3	4.0	3.98
DEML323	Ionized	3.5	0.20	2.4	3.98

Notes. Columns are: type of environment (Col. 2), hydrogen column density (H/cm²) in each phase of the gas (Cols. 3–5), and electron density in cm⁻³ (Col. 6).^(★) Following Paradis et al. (2011a).

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