Search for brown-dwarf companions of stars | Astronomy & Astrophysics (A&A)

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201015427e]

Table 3

Single-companion Keplerian orbital solutions of the surveyed stars.

Object	γ_C98	γ_C07	P	e	K₁	T₀	ω
	(km s^-1)	(km s^-1)	(day)		(m s^-1)	(JD^⋆)	(deg)

HD 3277
HD 17289
HD 30501
HD 43848^g
HD 43848^h
HD 52756
HD 53680
HD 74014
HD 89707
HD 154697
HD 164427A
HD 167665
HD 189310
HIP 103019	^b	···

HD 4747^d			7900^a
HD 4747^e	^c
HD 4747^f			29000^a
HD 211847^d	6.689^a	6.689^a	3750^a
HD 211847^e	6.689^a	6.689^a
HD 211847^f	6.689^a	6.689^a	100000^a

Notes.

^(a)

Fixed.

^(b)

HARPS systemic velocity.

^(c)

KECK HIRES systemic velocity is km s^-1.

^(d)

Lower period limit.

^(e)

Best-fit solution.

^(f)

Upper period limit.

^(g)

Final solution at lower eccentricity. The MIKE systemic velocity is km s^-1.

^(h)

Formal solution at higher eccentricity. The MIKE systemic velocity is km s^-1.

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