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Table A.3

Physical parameters obtained by fitting the NH3 spectra between 23-25 GHz.

Label Rp (au) size (″) VLSR (km s−1) FWHM (km s−1) Tex (K) NNH3 (1016 cm−2) τ55(c)
(1) (2) (3) (4) (5) (6) (7) (8)
Eastern: +380 0.452(a) −8.1±0.1 7.5±0.3 18310+11$\[183_{-10}^{+11}\]$ 7.080.31+0.25$\[7.08_{-0.31}^{+0.25}\]$ 0.2
Western: −380 0.452(a) −4.3±0.1 3.9±0.2 16512+11$\[165_{-12}^{+11}\]$ 3.980.17+0.24$\[3.98_{-0.17}^{+0.24}\]$ 0.2
Central: (b) 0 0.452 −4.1±0.2 4.1±0.8 17613+15$\[176_{-13}^{+15}\]$ 0.210.02+0.03$\[0.21_{-0.02}^{+0.03}\]$ 0.01
0 0.452 +1.2±0.2 5.0±0.8 21616+16$\[216_{-16}^{+16}\]$ 0.350.04+0.05$\[0.35_{-0.04}^{+0.05}\]$ 0.01

Notes. Columns 1 to 3: Pointing position with reference to Fig. 3, sky projected distance from the star, and extent of integrated spectra, respectively. Columns 4 and 5: Combined LSR velocity and FWHM of the NH3 para lines with uncertainties, the former to be compared with a systemic velocity of −4.5 km s−1. Columns 6 and 7: Excitation (and kinetic) temperature and column density of NH3 gas modelled with MCWeeds (with fitted uncertainties). Column 8: Opacity of the NH3 (5, 5) line. (a)Extended emission. (b)Composition of two velocity components, one per line. (c)We explicitly note that all fitted components are optically thin.

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