Orientation of the rotation axis and the location of water-ice sublimation activity of the main-belt comet 313P/Gibbs

Open Access

Fig. 10

Residual for FWHM of the dust tail between the simulation results and the observational image vs. local latitude. The dashed blue line corresponds to an ecliptic longitude of a rotation axis of 70^°, with the local latitude ranging from 40^° to 90^°. The solid red line corresponds to an ecliptic longitude of 250^°, with the local latitude ranging from −40^° to −90^°.

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