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Table D.2.

Parameters of observed, massive (near-)contact systems in the Magellanic Clouds.

Name p(d) q = M2/M1 M(M) R(R) Teff(kK) R/RRL Reference
VFTS 352 1.124 0.99(0.01) 28.85(0.30) 7.25(0.02) 41.45(1.17 : 0.80) 1.01 A21
28.63(0.30) 7.22(0.02) 44.15(1.1 : 1.2) 1.08
VFTS 066 1.141 0.52(0.05) 13.0(7.0 : 5.0) 5.8(0.5 : 0.8) 32.8(1.7 : 1.0) 1.07 M20
6.6(3.5 : 2.8) 4.4(0.4 : 0.8) 29.0(1.0 : 1.2) 1.09
VFTS 661 1.266 0.71(0.02) 27.3(0.9 : 1.0) 6.80(0.04 : 0.01) 38.4(0.9 : 0.4) 0.94 M20
19.4(0.6 : 0.7) 5.70(0.03 : 0.01) 31.8(1.4 : 0.6) 0.92
VFTS 217 1.855 0.83(0.01) 46.8(11.7) 10.1(1.5 : 1.2) 45.0(0.6 : 0.4) 0.91 M20
38.9(9.7) 9.4(1.4 : 1.0) 41.8(1.7 : 0.6) 0.92
VFTS 563 1.217 0.76(0.01) 26.2(11.9 : 52) 6.6(0.4 : 0.7) 32.4(1.0 : 0.9) 0.95 M20
20.0(9.1 : 3.9) 5.8(0.4 : 0.6) 32.4(1.2 : 0.9) 0.95
MACHO CB 1.217 0.64(0.01) 41.2(1.2) 9.56(0.02) 50 1.06 O01
27.0(1.2) 7.99(0.05) 49.5 1.09
SMC 108086 0.883 0.85(0.11) 16.9(1.2) 5.7(0.2) 36.00(0.69 : 0.66) 1.19 A21
14.3(1.7) 5.3(0.2) 35.20(0.64 : 072) 1.19

Notes For each system, the first (second) line gives the mass, radius, effective temperature and relative overflow for the primary (secondary).

References A21: Abdul-Masih et al. (2021); M20: Mahy et al. (2020a); O01: Ostrov (2001) MACHO* J053441.3-693139 OGLE SMC-SC10 108086

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