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Fig. 5.


Peculiar motion of 1FGL J1018.6–5856 on its regional standard of rest (RSR) as a function of the distance between the Sun and the source. The orange lines show the average velocity whereas the colored region represents the 1-σ confidence interval. We show the components in the direction to the Galactic center (ux), to the Galactic rotation (uy), and towards the Galactic north pole (uz). The bottom panel shows the module of the peculiar motion (|u|). The vertical blue lines represent the average distance to 1FGL J1018.6–5856 (solid line) and its ±1-σ confidence interval (dashed lines).

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