Since we see on the spectra of the pixels corresponding to the strong source a continuum between 5.15 and 5.5 µm that we attribute to the photospheric emission of the exciting star (see Fig. 3)
Since we see on the spectra of the pixels corresponding to the strong source a continuum between 5.15 and 5.5 µm that we attribute to the photospheric emission of the exciting star (see Fig. 3)