Binary orbital evolution driven by a circumbinary disc

Free Access

Table 1.

Summary of the physical parameters for the standard model.

q	α	h	r_in	r_out
0.5	0.1	0.1	2.5	6.0

Notes. The values are the binary star mass ratio q = M₂/M₁, the disc viscosity α, the aspect ratio h, and the initial radial extent of the disc r_in, r_out (see Eqs. (10) and (11)).

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.