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Table 1:

Revised astrophysical parameters and orbital elements of EBS showing apsidal motion.

System
P (d) Mass Radius $T_{\rm eff}$ $\log g$ e d$\omega$/dt Ref.
  (days) ($M_{\odot}$) ($R_{\odot}$) (K) (cgs)   (deg/cycle)  
EM Car 3.41 22.83 $\pm$ 0.32 9.35 $\pm$ 0.17 34 000 $\pm$ 2000 3.855 $\pm$ 0.016 0.0120 $\pm$ 0.0005 0.081 $\pm$ 0.005 1
    21.38 $\pm$ 0.33 8.35 $\pm$ 0.16 34 000 $\pm$ 2000 3.925 $\pm$ 0.016      

V478 Cyg

2.88 16.62 $\pm$ 0.33 7.428 $\pm$ 0.072 30479 $\pm$ 1000 3.9173 $\pm$ 0.0074 0.0158 $\pm$ 0.007 0.1047 $\pm$ 0.0010 2, 3, 4
    16.27 $\pm$ 0.33 7.428 $\pm$ 0.072 30549 $\pm$ 1000 3.9080 $\pm$ 0.0075      

V453 Cyg

3.89 13.82 $\pm$ 0.35 8.447 $\pm$ 0.068 27800 $\pm$ 400 3.7253 $\pm$ 0.0056 0.022 $\pm$ 0.002 0.054 $\pm$ 0.003 3, 5, 6,7
    10.64 $\pm$ 0.22 5.422 $\pm$ 0.068 26200 $\pm$ 500 3.9970 $\pm$ 0.0095      

CW Cep

2.73 13.05 $\pm$ 0.20 5.65 $\pm$ 0.12 28300 $\pm$ 1000 4.050 $\pm$ 0.019 0.0293 $\pm$ 0.0006 0.0582 $\pm$ 0.0005 4, 8, 9, 10
    11.91 $\pm$ 0.20 5.14 $\pm$ 0.12 27700 $\pm$ 1000 4.092 $\pm$ 0.021      

QX Car

4.48 9.24 $\pm$ 0.12 4.292 $\pm$ 0.091 23800 $\pm$ 500 4.139 $\pm$ 0.018 0.278 $\pm$ 0.003 0.01222 $\pm$ 0.00022 11, 12
    8.46 $\pm$ 0.12 4.054 $\pm$ 0.091 22600 $\pm$ 500 4.150 $\pm$ 0.019      

V539 Ara

3.17 6.240 $\pm$ 0.066 4.517 $\pm$ 0.084 18100 $\pm$ 500 3.924 $\pm$ 0.016 0.053 $\pm$ 0.001 0.0193 $\pm$ 0.0010 13, 14, 15
    5.314 $\pm$ 0.060 3.429 $\pm$ 0.083 17100 $\pm$ 500 4.094 $\pm$ 0.021      

AG Per

2.03 5.35 $\pm$ 0.16 2.996 $\pm$ 0.071 18200 $\pm$ 800 4.213 $\pm$ 0.020 0.0709 $\pm$ 0.0006 0.0262 $\pm$ 0.0004 4, 16
    4.89 $\pm$ 0.13 2.606 $\pm$ 0.070 17400 $\pm$ 800 4.296 $\pm$ 0.023      

U Oph

1.68 5.273 $\pm$ 0.091 3.485 $\pm$ 0.021 16 440 $\pm$ 250 4.0759 $\pm$ 0.0043 0.00305 $\pm$ 0.00008 0.07919 $\pm$ 0.00001 17, 18
    4.739 $\pm$ 0.072 3.111 $\pm$ 0.034 15590 $\pm$ 250 4.1282 $\pm$ 0.0087      

V760 Sco

1.73 4.969 $\pm$ 0.090 3.016 $\pm$ 0.066 16900 $\pm$ 500 4.176 $\pm$ 0.019 0.0270 $\pm$ 0.0005 0.0443 $\pm$ 0.0004 19, 20
    4.609 $\pm$ 0.073 2.642 $\pm$ 0.066 16300 $\pm$ 500 4.258 $\pm$ 0.021      

GG Lup

1.85 4.106 $\pm$ 0.044 2.381 $\pm$ 0.025 14750 $\pm$ 450 4.2983 $\pm$ 0.0089 0.150 $\pm$ 0.005 0.0181 $\pm$ 0.0006 21
    2.504 $\pm$ 0.023 1.726 $\pm$ 0.019 11000 $\pm$ 600 4.3628 $\pm$ 0.0092      

$\zeta$ Phe

1.67 3.921 $\pm$ 0.045 2.853 $\pm$ 0.015 14400 $\pm$ 800 4.1210 $\pm$ 0.0040 0.0113 $\pm$ 0.0010 0.0280 $\pm$ 0.0010 13, 22
    2.545 $\pm$ 0.026 1.854 $\pm$ 0.011 12 000 $\pm$ 600 4.3076 $\pm$ 0.0046      

IQ Per

1.74 3.504 $\pm$ 0.054 2.446 $\pm$ 0.024 12300 $\pm$ 230 4.2060 $\pm$ 0.0080 0.0763 $\pm$ 0.0008 0.0138 $\pm$ 0.0003 4, 23
    1.730 $\pm$ 0.025 1.499 $\pm$ 0.016 7700 $\pm$ 140 4.3248 $\pm$ 0.0085      

PV Cas

1.75 2.816 $\pm$ 0.050 2.301 $\pm$ 0.020 10200 $\pm$ 250 4.1640 $\pm$ 0.0063 0.0322 $\pm$ 0.0005 0.0190 $\pm$ 0.0004 24, 25, 26
    2.757 $\pm$ 0.054 2.258 $\pm$ 0.019 10190 $\pm$ 250 4.1713 $\pm$ 0.0067      

V451 Oph

2.20 2.769 $\pm$ 0.062 2.642 $\pm$ 0.031 10800 $\pm$ 800 4.0368 $\pm$ 0.0091 0.0125 $\pm$ 0.0015 0.0120 $\pm$ 0.0007 27
    2.351 $\pm$ 0.052 2.029 $\pm$ 0.028 9800 $\pm$ 500 4.195 $\pm$ 0.011      

V1647 Sgr

3.28 2.184 $\pm$ 0.037 1.832 $\pm$ 0.018 9600 $\pm$ 300 4.2517 $\pm$ 0.0078 0.4130 $\pm$ 0.0005 0.00546 $\pm$ 0.00006 28
    1.967 $\pm$ 0.033 1.668 $\pm$ 0.017 9100 $\pm$ 300 4.2879 $\pm$ 0.0084      

EK Cep

4.43 2.025 $\pm$ 0.023 1.5801 $\pm$ 0.0065 9000 $\pm$ 200 4.3473 $\pm$ 0.0027 0.109 $\pm$ 0.003 0.00093 $\pm$ 0.00010 29, 30, 31, 33
    1.122 $\pm$ 0.012 1.3156 $\pm$ 0.0057 5700 $\pm$ 200 4.2499 $\pm$ 0.0032      

IT Cas

3.90 1.3315 $\pm$ 0.0093 1.595 $\pm$ 0.018 6470 $\pm$ 100 4.1574 $\pm$ 0.0096 0.0797 $\pm$ 0.0016 0.00117 $\pm$ 0.00007 32, 33
    1.3290 $\pm$ 0.0078 1.563 $\pm$ 0.018 6470 $\pm$ 100 4.1740 $\pm$ 0.0097      

V636 Cen

4.28 1.0518 $\pm$ 0.0048 1.0188 $\pm$ 0.0043 5900 $\pm$ 85 4.4441 $\pm$ 0.0036 0.1348 $\pm$ 0.0012 0.00080 $\pm$ 0.00005 34
    0.8545 $\pm$ 0.0030 0.8302 $\pm$ 0.0043 5000 $\pm$ 100 4.5317 $\pm$ 0.0044      

References. 1 Andersen & Clausen (1989); 2 Popper & Etzel (1981); 3 Popper & Hill (1991); 4 Wolf et al. (2006); 5 Southworth et al. (2004); 6 Pavlovski & Southworth (2009); 7 Wachmann (1974); 8 Popper (1974); 9 Clausen & Giménez (1991); 10 Stickland et al. (1992); 11 Andersen et al. (1983); 12 Giménez et al. (1986); 13 Andersen (1983); 14 Clausen (1996); 15 Wolf & Zejda (2005); 16 Giménez & Clausen (1994); 17 Holmgren et al. ( 1991); 18 Vaz et al. (2007); 19 Andersen et al. (1985); 20 Wolf (2000); 21 Andersen et al. (1993); 22 Zasche & Wolf (2007); 23 Lacy & Frueh (1985); 24 Popper (1987a); 25 Barembaum & Etzel (1995); 26 Svarícek et al. (2008); 27 Clausen et al. (1986); 28 Andersen & Giménez (1985); 29 Popper (1987b); 30 Martin & Rebolo (1993); 31 Claret et al. (1995); 32 Lacy et al. (1997); 33 Wolf et al. (2009); 34 Clausen et al. (2009).


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