Fig. 10.
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2D distribution of the ∼24 OB+NS binaries of our fiducial synthetic SMC population in the orbital period – eccentricity plane. The number in each pixel is colour-coded. The 7 SMC BeXBs with eccentricity measurements (Townsend et al. 2011; Coe & Kirk 2015) are indicated by black diamonds. The B star + radio pulsar binary (Kaspi et al. 1994; Bell et al. 1995) is marked by a black star, the supergiant X-ray binary SMC X-1 by a black triangle (Falanga et al. 2015).
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