Cyclic variability of the accretion disk in the eclipsing binary OGLE-LMC-DPV-065

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Table 5.

Light curve fit parameters for the data segments.

Set	F_d	T_disk	A_hs	θ_hs	λ_hs	θ_rad	A_bs	θ_bs	λ_bs	a_T	R_disk	d_e	d_c
	±0.01	±60	±0.04	±1.2	±3.0	±3.0	±0.04	±1.3	±8.0	±0.02	±0.1	±0.1	±0.2
		(K)		(°)	(°)	(°)		(°)	(°)		(R_⊙)	(R_⊙)	(R_⊙)
1	0.864	9802	1.24	21.2	306.0	−20.8	1.28	38.7	67.0	0.73	22.77	4.83	3.20
2	0.782	9298	1.38	20.9	307.7	−35.5	1.48	30.5	60.7	0.58	20.61	4.21	5.47
3	0.748	9826	1.37	21.4	311.1	−32.2	1.31	28.9	85.2	0.36	19.73	6.35	7.55
4	0.813	7710	1.11	19.6	316.2	−0.5	1.30	27.7	189.2	0.72	21.43	6.72	3.18
5	0.439	7089	1.34	21.4	307.1	−29.9	1.30	41.1	80.4	0.65	11.58	6.25	3.19
6	0.400	6436	1.47	21.3	328.6	−34.6	1.36	43.6	108.2	0.64	10.55	5.73	4.67
7	0.493	6772	1.39	20.8	306.3	−37.0	1.56	47.9	118.4	0.53	12.99	5.33	7.27
8	0.629	7355	1.34	21.1	307.1	−33.9	1.47	54.7	127.9	0.71	16.60	5.54	5.57
9	0.732	7646	1.12	23.3	308.4	−36.5	1.43	26.5	109.6	0.50	19.31	4.43	6.95
10	0.623	8785	1.21	21.3	306.7	−36.6	1.40	30.0	75.0	0.74	16.44	5.61	5.79
11	0.740	8790	1.20	20.6	309.1	−36.4	1.35	28.8	92.5	0.74	19.50	5.16	7.57
12	0.959	6821	1.14	19.8	339.5	−1.3	1.33	31.3	141.0	0.58	25.28	5.14	4.68
13	0.952	6592	1.11	21.6	311.0	−35.8	1.36	33.3	151.9	0.68	25.11	5.68	5.37
14	0.943	5179	1.26	21.6	313.2	−36.3	1.57	53.4	157.8	0.35	24.88	4.39	6.07
15	0.861	5622	1.13	19.4	338.0	−31.8	1.52	50.4	157.6	0.35	22.72	4.63	6.06
16	0.990	5482	1.39	21.0	351.5	−35.4	1.50	53.1	132.4	0.50	26.09	2.83	6.13
17	0.796	6853	1.23	20.8	329.0	−35.8	1.51	35.7	113.4	0.67	20.99	4.32	4.23
18	0.803	8240	1.33	21.6	316.2	−35.0	1.41	29.0	68.4	0.47	21.19	3.36	4.09
19	0.717	9881	1.53	21.4	313.7	−26.3	1.43	54.3	64.1	0.30	18.92	4.16	3.93
20	0.790	9774	1.39	21.5	308.0	−25.4	1.52	30.5	82.4	0.35	20.82	3.52	1.23

Mean	0.754	7698	1.28	21.1	317.7	−29.8	1.42	38.5	109.2	0.56	19.88	4.91	5.11
std	0.168	1530	0.13	0.8	13.3	10.8	0.09	10.3	37.2	0.15	4.42	1.03	1.68

Notes. The disk radius derived from F_d is also shown. Mean and standard deviation are also given along with formal errors (see text for details).

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