Open Access

Fig. 9.

image

Download original image

Gamma-ray peak separations (Δ) vs. radio/gamma-ray phase-lag δg − r for gamma-ray pulsars from 3PC (coloured markers) and the MSPs studied here (black stars). For two pulsars, the definition of the primary gamma-ray peak is potentially ambiguous, and so for these we show the alternative values with empty markers, linked by dashed lines. Pulsars with only one gamma-ray peak are shown below Δ = 0 with a random scatter in the y-axis for clarity.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.