Relativistic apsidal motion in eccentric eclipsing binaries

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Table 3:

Adopted masses of the selected EEB and their classical and relativistic apsidal motion.
System	Spectral	M₁	M₂	$\dot{\omega}_{\rm rel}$	$\dot{\omega}_{\rm obs}$	$\dot{\omega}_{\rm rel} / \dot{\omega}_{\rm obs}$	Source
	type	[ $M_{\odot}$ ]	[ $M_{\odot}$ ]	[10^-5 deg/cycle]		[%]
BW Aqr	F7V	1.49(2)	1.39(2)	32	92	35	Clausen (1991)
V889 Aql*	B9.5V+A0V	2.4	2.2	25	45	78	Wolf et al. (2005)
SW CMa	A3	2.22	2.03	34	67	51	Clausen et al. (2008)
IT Cas	F6V+F6V	1.330(9)	1.328(8)	40	87	46	Lacy et al. (1997)
V459 Cas	A1V+A1V	2.02(3)	1.96(3)	33	71	46	Lacy et al. (2004)
V636 Cen	F8/G0V	1.04	0.85	32	80	40	Clausen et al. (2008)
EK Cep	A1V+G5V	2.029(23)	1.124(12)	44	93	47	Popper (1987)
V731 Cep	B8.5V+A1.5V	2.577(98)	2.017(84)	45	60	75	Bakis et al. (2008)
TV Cet*	F2V+F5V	1.39	1.27	24	30	80	Wolf et al. (2001)
V541 Cyg	B9.5V+B9.5V	2.24(9)	2.24(8)	32	32	100	Lacy (1998)
V1143 Cyg	F5V+F5V	1.391(16)	1.347(13)	39	72	54	Andersen et al. (1987)
V1147 Cyg	A2	2.15	2.01	24	40	60	Wetterer et al. (2006)
BF Dra	F8V+F8V	1.4(1)	1.4(1)	25	56	45	Imbert (1985)
RW Lac*	G5V+G7V	0.928(6)	0.870(4)	17	18	97	Lacy et al. (2005)
V345 Lac	B8V+B8V	3.0	3.0	59	107	55	Wolf et al. (2004)
RR Lyn*	A2IV+F0V	1.89(7)	1.49(5)	27	40	67	Khaliullin & Khaliullina (2002)
EW Ori	G0V+G5V	1.190(14)	1.154(14)	27	57	47	Popper et al. (1986)
GG Ori	B9.5V+B9.5V	2.342(16)	2.338(17)	45	57	79	Torres et al. (2000)
VV Pyx	A1V+A1V	2.098(18)	2.098(18)	51	138	37	Andersen et al. (1984)
V1094 Tau*	G0V+G3V	1.10(1)	1.01(1)	22	65	34	Griffin & Boffin (2003)

Note: * possible triple system.

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