The formation of black holes in non-interacting isolated binaries - Gaia black holes as calibrators of stellar winds from massive stars

Open Access

Table D.1.

Counts of systems in the MW for different selections on the BH mass (M₁), the companion mass (M₂), the orbital period (P_orb), and the eccentricity (e). The two simulations (sim1 and sim2) are the ones shown in Figs. 5 and C.1, respectively.

M₁[M_⊙]	M₂[M_⊙]	P_orb[d]	e	sim1	sim2
all	all	all	all	$5805_{- 5805}^{+ 19156}$ $5805^{+19156}_{-5805}$	$2619_{- 2619}^{+ 8643}$ $2619^{+8643}_{-2619}$
[9.5, 10.5]	[0.50, 2.00]	[100.00,300.0]	all	$9_{- 9}^{+ 31}$ $\phantom{000}9^{+31\phantom{000}}_{-9}$	$50_{- 50}^{+ 166}$ $\phantom{00}50^{+166\phantom{0}}_{-50}$
[8.6,9.8]	[0.88, 1.26]	[185.54, 1277.3]	[0.446, 0.5185]	$6_{- 6}^{+ 19}$ $\phantom{000}6^{+19\phantom{000}}_{-6}$	$4_{- 4}^{+ 13}$ $\phantom{000}4^{+13\phantom{000}}_{-4}$
all	all	< 5 000	all	$1391_{- 1391}^{+ 4592}$ $1391^{+4592\phantom{0}}_{-1391}$	$1293_{- 1293}^{+ 4267}$ $1293^{+4267}_{-1293}$
[8.6,9.8]	[0.88, 1.26]	all	all	$429_{- 429}^{+ 1414}$ $\phantom{0}429^{+1414\phantom{0}}_{-429}$	$146_{- 146}^{+ 482}$ $\phantom{0}146^{+482\phantom{0}}_{-146}$
[8.6,9.8]	[0.88, 1.26]	< 5 000	all	$123_{- 123}^{+ 406}$ $\phantom{0}123^{+406\phantom{00}}_{-123}$	$100_{- 100}^{+ 331}$ $\phantom{0}100^{+331\phantom{0}}_{-100}$

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