... The estimated extinction of the source is AV 14, and a precise position following from the detection of the radio counterpart allowed us to identify this source as a K = 15 infrared source (Marti et al. ...
... In other words, we suggest that localization of "BB" bump feature emission should be better identified during the direct observation of the innermost source region near the compact object (CC). ...
... As a result, the implementation of the phenomenological powerlaw model makes much harder, or even impossible to correctly identify the spectral state of the source, which is an imminent task for our study. ...