Fig. 10.
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Fit of the infrared extinction AKs between 5 and 15 kpc from Marshall et al. (2006) with a linear function (the best-fit line and the lines taking into account the associated errors are in blue). The red horizontal lines represent the estimate with the corresponding upper and lower limits of AKs from Eq. (3). The distance to the source is thus d = 7.6 ± 1.1 kpc.
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