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Table 1.

Stellar parameters for the B+BH and strB+Be scenario used for our simulations of the LB-1 system, and as found in the literature.

B+BH
strB+Be
Reference This work (1) (2) This work (3) (2)
Primary Type B star B star B star Stripped star Stripped star Stripped star
14 ∈[13.5,14.5] ∈[15.0,15.6] 12.7 12.7 ∈[12.4,12.6]
5.3 ∈[4.1,6.5] ∈[5.4,6.7] 5.4 5.4 ∈[4.4,5.3]
4.2 ∈[1.3,5.5] ∈[3.8,7.0] 1.3 ∈[1.1,1.9] ∈[0.5,1.3]
log g(1) 3.5 ∈[3.35,3.65] ∈[3.4,3.8] 3.1 3.0 ∈[2.8,3.2]
21 < 27(b) 21(c) 11 ∈[13, 30] 11
0.1 0.1 0.1 0.2 0.21 0.2


Secondary Type BH BH Be star Be star Be star
18 18 ∈[18.7,19.1]
1 3.7 3.7 ∈[2.8,3.4]
30 ∈[13,30] 7 ∈[5,9] ∈[1.6,6.9]
log g(2) 4.15 4.0 ∈[3.7,4.3]
600 ∈[400, 560] 480
0.1 0.08 0.1

Notes. The values for the rotational velocities have been deduced from the inclination used in this paper (see Table 2, i = 22° and i = 39° for the B+BH and strB+Be scenarios, respectively). For consistency, we calculated log g from the stellar radii and masses.

References. (1) Simón-Díaz et al. (2020); (2) Lennon et al. (2021); (3) Shenar et al. (2020).

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