Ap stars with resolved magnetically split lines: Magnetic field determinations from Stokes I and V spectra

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Table 12

New or revised orbital elements of spectroscopic binaries. The second row for each entry gives its standard deviation.


HD/HDE	P _orb	T ₀	e	V ₀	ω	K	f(M)	a sini	N	O−C
	(d)	(HJD)		(km s^-1)	(°)	(km s^-1)	(M_⊙)	(10⁶ km)		(km s^-1)


9996	272.81	2 444 492.8	0.512	0.36	19.5	11.51	0.0273	37.1	57	1.37
	0.15	2.0	0.021	0.19	3.1	0.28	0.0024	1.1
12288	1546.5	2 444 488.3	0.342	−53.29	122.5	9.16	0.102	183.1	59	0.65
	4.6	9.3	0.013	0.11	3.4	0.15	0.051	3.2
29578	926.7	2 449 148.3	0.377	15.66	225.3	9.74	0.070	115.0	27	0.60
	2.8	8.1	0.018	0.14	8.1	0.28	0.021	3.4
50169	1764	2 448 529	0.47	13.35	44.3	1.90	0.0009	40.7	42	0.51
	49	36	0.10	0.12	9.1	0.32	0.0223	7.4
55719	46.31803	2 441 672.98	0.1459	−6.46	195.0	48.27	0.522	30.42	76	2.15
	0.00078	0.38	0.0071	0.25	3.0	0.37	0.012	0.24
61468	27.2728	2 445 994.20	0.1723	32.04	181.7	19.35	0.1309	13.47	20	0.61
	0.0014	0.29	0.0057	0.17	2.2	0.14	0.0029	0.29
94660	848.96	2 445 628.6	0.4476	18.53	264.5	17.94	0.3631	187.3	47	0.36
	0.13	1.7	0.0049	0.06	0.8	0.11	0.0075	1.2
116458	126.233	2 441 422.3	0.143	2.68	70.7	14.13	0.0357	24.27	65	1.08
	0.012	2.1	0.014	0.15	6.4	0.19	0.0015	0.33
187474	689.68	2 435 139.0	0.4856	−1.771	7.1	11.06	0.0646	91.7	108	0.75
	0.10	2.3	0.0092	0.074	1.3	0.14	0.0027	1.2

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