Characterization of Kepler early-type targets | Astronomy & Astrophysics (A&A)

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Table 6:

Spectroscopic binaries and stars with possible RV variations.
HIP	RV [km s^-1]	RV [km s^-1]	Ref.	var
	this paper	literature
92637	-22.0 $\pm$ 2.8	27 $\pm$ 36	(1)	SB1?
96277	-0.52 $\pm$ 1.16^a	...	...	?
96299 A	-7.77 $\pm$ 1.22	...	...	SB2
96299 B	45.13 $\pm$ 1.26	...	...	...
96762	16.51 $\pm$ 1.10	24 $\pm$ 6.2	(2)	SB1?
97254	-4.28 $\pm$ 6.19	-23 $\pm$ 1.5	(2)	SB1
97724	-14.76 $\pm$ 4.05	-31 $\pm$ 3.4	(2)	SB1
98551 A	-23.44 $\pm$ 3.29	...	...	SB2
98551 B	44.64 $\pm$ 1.97	...	...	...
98814	-40.70 $\pm$ 3.51	$\gamma = 8$	(4)	SB1

Notes. ^(a) Mean of the three RV values reported in Table 3. (1) Dworetsky et al. (1982); (2) Fehrenbach & Burnage (1990); (3) Fehrenbach et al. (1997); (4) Struve (1946).

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