Unveiling the nature and fate of the almost-dark cloud AGC 226178 through H I mapping

Open Access

Fig. 6.

The H I column density radial profile of the natural-weighted VLA image of AGC 226178. The dark blue represents the Gaussian fit to the profile, whereas the light blue represents the deconvolved intrinsic profile. The red dashed line indicates the 3σ detection limit, whereas the grey solid line is the beam profile.

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