Fig. 1
Schematic representation of the supermassive binary system Eta Carinae. Electrons (e) and hadrons (p) can be accelerated on both shocks to different maximum energies due to different conditions at the shocks from the sides of the Eta Carinae star and the companion star. The details of the considered scenario are given in the main text of the paper.
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.