Fig. 3.
Calculated spectrum of PSR B1259–63/LS 2883 at periastron (i.e. ϕ = 0, dashed lines) and the disc passage after periastron (i.e. ϕ = ϕd, solid lines). The Swift observational data are taken from Chernyakova et al. (2014) at 23.96 days after periastron, and the H.E.S.S. observational data are taken from the preliminary data reported by Romoli et al. (2017).
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.