The Gaia-ESO Survey: Dynamical analysis of the L1688 region in Ophiuchus

E. Rigliaco; B. Wilking; M. R. Meyer; R. D. Jeffries; M. Cottaar; A. Frasca; N. J. Wright; A. Bayo; R. Bonito; F. Damiani; R. J. Jackson; F. Jiménez-Esteban; V. M. Kalari; A. Klutsch; A. C. Lanzafame; G. Sacco; G. Gilmore; S. Randich; E. J. Alfaro; A. Bragaglia; M. T. Costado; E. Franciosini; C. Lardo; L. Monaco; L. Morbidelli; L. Prisinzano; S. G. Sousa; S. Zaggia

doi:10.1051/0004-6361/201527253

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Volume 588 (April 2016)

A&A, 588 (2016) A123

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Table 3

Confirmed members without stellar parameters recommended by GES.

CNAME	RA	Dec	L _star ^a	Mass^a	T _eff ^a	RV^b	W(Li) ^b	Source name^c
	hh:mm:ss		L_⊙	M_⊙	K	km s^-1	mÅ

16253958-2426349	16:25:39.58	−24:26:34.9	0.18	0.31	3499	−9.27 (2.00)	457.1 (20.0)	WLY 2−3
16263416-2423282	16:26:34.16	−24:23:28.2	1580	5.00	18967	−2.37 (2.71)	...	Oph S1
16282480-2435434	16:28:24.80	−24:35:43.4	0.03	0.14	2999	...	...	[WMR2005](3−39)
16284304-2422522	16:28:43.04	−24:22:52.2	0.06	0.15	3033	−0.01 (3.53)	757.6 (20.0)	[WMR2005](2−23)

Notes. The numbers in parentheses represent the errors on the measured quantities.

^(a)

Parameters from WMR05 (the values for the luminosity listed assumed a distance of 150 pc).

^(b)

Parameters from GES.

^(c)

Identification number as used by WMR05 in their Table 4.

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