Fig. 2
Planck maps of NGC 6369. An extended structure, marked by the arrows, appears to surround the PN, mostly visible in the HFI channels. This may constitute a hint for the presence of a dusty halo. However, the central component is well detected in several channels, allowing us to calculate its flux. The average FWHM of the effective beam is shown in the bottom-left corner of each map.
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