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Table 5

Parameters of the models for the three selected positions in the vicinity of Sgr A*.

Position D (b,c) D/G Source log Tk (c,d) O/P (c) 16O/18O V t (e) Td (e) log τd (f) log log
Com. (a) (kpc) Ratio (c) (%) Radius (d) (pc) (cm−3) (K) Ratio (c) (×10−6) (km s−1) (K) (cm−2) (cm−2)
CND1 1 7.9 1 0.31 4.5 200 3 250 9.3 23 ± 3 45 −2.1 22.48 17.45
                             
2 7.9 1 0.08 5.2 500 3 250 6.7 23 ± 3 30 −2.0 22.59 17.42
                             
CND2 1 7.9 1 0.32 4.5 175 3 250 1.3 14 ± 3 15 −2.1 22.50 16.62
                             
2 7.9 1 0.06 5.3 325 3 250 13.3 14 ± 3 25 −2.0 22.56 17.69
                             
20 km s−1 cloud 1 7.9 1 2.3 4.6 100 3 250 0.04 9 ± 2 26 (i) −1.1 23.44 16.04

Notes. (a) Component. (b) Distance to source. (c)Fixed parameter. (d)These values are taken from Requena-Torres et al. (2012) for the two CND positions. The and Tk are taken from Amo-Baladrón et al. (2011) and Hüttemeiser et al. (1993), respectively, for the 20 km s−1 cloud, while the radius of this source is estimated from our H2O maps (see Appendix B.2). (e)Free parameter. (f)Predicted value at 250 μm. The uncertainty in the τd is calculated assuming a 10% uncertainty in the source size. (g)Estimated assuming a mass-absorption coefficient of 8.2 cm2 g−1 at 250 μm (González-Alfonso et al. 2014) and a D/G of 1%. derived using the and given in this table. (i)The Td used for the 20 km s−1 position is fixed as no observational continuum was available to constrain the Td of this position.

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