Fig. 3
2-σ differential flux upper limits (red lines) of WR 147 compared to modelling explained in Reimer & Reimer (2009b). The model curves shown here correspond to a parameter set where a 30 G surface magnetic field for the B-star has been used. Black curves show IC spectra of WR 147 for possible geometric viewing angles ΘL = 10°, 20°, 30°, 40°, 50°, 60°, 90°, 120°, 150°, and 170° (lower to upper curve). We assume an inclination of i = 85° and a binary separation of d ≈ 4800 AU. The MAGIC upper limits (blue dotted lines) are taken from Aliu et al. (2008).
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.