Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [C ii] SOFIA/GREAT observations

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Table 3

Results from the Gaussian fit decomposition.

Region	A₁	A₂	B	I_{[C ii]}(CO)/I_{[C ii]}
	H i	H i	CO	central value	1σ interval

I-1	0.12 ± 0.08	0.06 ± 0.05	0.62 ± 0.10	77.4%	65−85%
I-2	0.04 ± 0.10	0.00 ± 0.04	0.70 ± 0.11	93.0%	85−100%
I-3	0.35 ± 0.04	0.04 ± 0.04	0.56 ± 0.08	34.3%	25−45%
II	0.29 ± 0.04	–	0.71 ± 0.06	49.5%	40−60%
III	0.29 ± 0.11	–	0.18 ± 0.24	17.5%	0−30%

Notes. A₁, A₂ and B are the coefficients of the components (Eq. (1)). Columns 5 and 6 list the central values and 1σ intervals of the fraction of [C ii] intensity associated with CO (see Sect. 3.2). The intensity fractions associated with H i are the remaining fraction of the [C ii] intensity.

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