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Fig. 11


From left to right, and from top to bottom: IRAC 8, 4.5 and 3.6 μm, and DSS-II (red band) images of the candidate bow-shock-producing star (star 8) embedded in the extended region of infrared emission (known as IRAS 17207 − 3404). The orientation and the scale of the images are the same.

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