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Fig. 13


SOAR Goodman spectrum of IGR J17329-2731, together with a model comprising an M giant star based on Phoenix models (Husser et al. 2013) plus an accretion disk. The model spectrum was reddened assuming E(BV) ~ 3. The inset shows the double-peaked Hα as seen in the high resolution spectrum, indicating the presence of an accretion disk around the compact object in IGR J17329-2731.

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