Table 1

Ranges of best-fit model parameters for the MWNSC in the Spitzer/IRAC 4.5 μm image, assuming constant fore- and background light.

Sérsic

Δx Δy Θ I e q n R e
(pc) (pc) (deg) (mJy arcsec-2) (pc)

Corrected [0.04,0.05] [− 0.20,0.03] [− 2.7, − 2.8] [1.5,4.9] [0.61,0.64] [1.0,3.5] [3.8,10.0] [1.11,1.20]
Symmetric [0.04,0.04] [− 0.10, − 0.10] [− 0.1, − 0.3] [0.8,4.9] [0.61,0.63] [1.2,3.7] [4.0,13.5] [1.57,1.64]

King

Δx Δy Θ I 0 q r c
(pc) (pc) (deg) (mJy arcsec-2) (pc)

Corrected [0.05,0.07] [− 0.26, − 0.10] [− 3.4, − 1.6] [16.4,37.6] [0.59,0.65] [1.7,3.2] [1.11,1.20] [
Symmetric [0.04,0.04] [− 0.10, − 0.10] [− 0.3, − 0.1] [16.4,30.6] [0.60,0.64] [1.9,3.6] [1.61,1.74]

Moffat

Δx Δy Θ I 0 q β
(pc) (pc) (deg) (mJy arcsec-2)

Corrected [− 0.03, − 0.00] [− 0.05, − 0.02] [− 3.6, − 1.1] [341,727] [0.59,0.62] [0.72,0.98] [1.22,1.36]
Symmetric [0.04,0.04] [− 0.10, − 0.10] [− 0.1, − 0.2] [359,725] [0.62,0.63] [0.71,0.95] [1.69,2.01]

Notes. The first line for each model refers to the PAH- and extinction-corrected image and the second line to the corrected and symmetrised image.

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