Free Access

Table C.1

Equalised assumptions for this research and the usual assumptions of the authors in the corresponding BPS codes.

binary_c Brussels code SeBa StarTrack This research

β (RLOF) Variable Conditional(1) Variable Conditional(1) 1
AML (RLOF) Isotropic re-emission Ring(2) () Orbit(2) (η = 2.5) Orbit(2) (η = 1) Orbit (η = 1)
CE(3) α (v2) α (v1) γα (T12) α (v1) α (v1)
αceλce/γ Variable(4) 1 2/1.75 1 1
Wind accretion B-H(5) No B-H(5) No(6) No
Tides Z77, H81, HTP02 Z77 PZV96 Z77, H81, HTP02, C07 No
Magn. braking RVJ83 No RVJ83 IT03 No

Notes.

(1)

Constant for non-degenerate accretors, variable for accretion onto a WD.

(2)

Except during accretion onto a compact object, AML = isotropic re-emission.

(3)

v1 = prescription Webbink (1984), v2 = prescription Hurley et al. (2002).

(4)

Based on detailed stellar structure models (Izzard 2004; Claeys et al. 2013).

(5)

B-H = Prescription based on Bondi & Hoyle (1944).

(6)

Wind accretion is taken into account for neutron star and black hole accretors assuming B-H-accretion.

Reference. T12 = Toonen et al. (2012); Z77 = Zahn (1977); H81 = Hut (1981); HTP02 = Hurley et al. (2002); PZV96 = Portegies Zwart & Verbunt (1996); C07 = Claret (2007); RVJ83 = Rappaport et al. (1983); IT03 = Ivanova & Taam (2003).

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.