Measuring spin in coalescing binaries of neutron stars that show double precursors

Open Access

Fig. 5.

Derived spin of the primary (Eq. (24)) for double-precursor events with various EOSs in binaries with fixed total masses of 2.5 M_⊙ and 2.8 M_⊙ as functions of mass ratio q. Solid lines represent Eq. (25).

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.