Relativistic apsidal motion in eccentric eclipsing binaries

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Table 1:

Apsidal-motion elements for ten selected eclipsing systems.
System	T₀	$P_{\rm s}$	e	$\dot{\omega}$	$\omega_0$	U
	[HJD-2400000]	[days]	-	[deg $\:\rm {cycle^{-1}}$ ]	[deg]	[10³ years]
IT Cas	45167.4167(3)	3.8966487(2)	0.0896(4)	0.00087(7)	331.2	4.4
V459 Cas	52565.6385(4)	8.4582621(8)	0.0244(2)	0.00071(8)	240.1	11.7
V541 Cyg	44881.7927(3)	15.3378983(7)	0.4736(5)	0.00032(6)	262.7	47.1
V1143 Cyg	42213.4335(5)	7.6407418(8)	0.535(4)	0.00072(8)	47.7	10.5
V1147 Cyg	50759.4353(6)	15.2513238(5)	0.276(1)	0.00040(5)	51.6	37.6
BF Dra	47276.3384(8)	11.210980(1)	0.3898(7)	0.00056(8)	93.2	19.7
V345 Lac	50200.7695(6)	7.4919003(2)	0.4568(8)	0.00107(8)	241.2	6,9
EW Ori	44948.0037(5)	6.9368439(7)	0.068(1)	0.00057(4)	314.1	12.0
GG Ori	47814.2022(5)	6.6314924(8)	0.220(1)	0.00057(6)	122.9	11.5
V1094 Tau	49702.4468(3)	8.9885451(5)	0.2667(5)	0.00065(7)	333.8	13.6

Source LaTeX | All tables | In the text

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