Free Access

Fig. 1


Main stages of the evolution of the binary system leading to the currently observed PSR J16142230, accompanied by a 0.5 M WD (detailed description in Sect. 2.1). A – main sequence stage; B – common envelope stage (secondary inside the primary); C – the primary becoming a He star; D – core-collapse supernova explosion of the primary; E – intermediate-mass X-ray binary stage, with a very strong mass loss; F – LMXB, NS recycling stage via accretion disk, secondary mass loss via RLO; G – current state, wide binary MSP+WD.

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.