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Fig. 4

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Spectral energy distribution of the progenitor of BLG-360. Symbols: observational data from OGLE-III, 2MASS, and MSX, as well as upper limits from IRAS (see text for more details). Vertical error bars: estimated uncertainties of the measurements. Horizontal error bars: photometric band widths used in the observations. Full curve: model spectrum obtained with the values of the model parameters listed in the first row of Table 1. Dashed curves: individual contributions of the star and the dusty envelope.

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