Open clusters in APOGEE and GALAH - Combining Gaia and ground-based spectroscopic surveys

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Table 3.

Properties of the 14 OCs in common between GALAH DR2 and Cantat-Gaudin et al. (2018).

Cluster	Star	RV	σ_RV	e_RV	⟨v sin i⟩^astar	Nr	RV_GDR2^b	σ_GDR2	Nr_GDR2	[Fe/H]	σ_[Fe/H]	e_[Fe/H]	Nr	[Fe/H]_lit	σ_[Fe/H],lit	Nr_lit	Ref.
	type	(km s⁻¹)					(km s⁻¹)			(dex)				(dex)
Alessi 24	MS	10.44		0.11	11.63	1	12.32	2.24	14	−0.13		0.07	1
Alessi 9	MS	−5.64		0.11	5.70	1	−6.44	1.14	39	−0.06		0.07	1
Alessi-Teutsch 12	MS	−11.00		0.12	5.35	1	−5.88	3.54	6	0.40		0.08	1
ASCC 16	MS	22.01		0.17	38.82^c	1	23.18	3.40	15	−0.08^d		0.06	1
ASCC 21	MS	20.05		1.06	19.99^c	1	18.70	4.45	9	−0.13^d		0.08	1
Collinder 135	MS	17.08	0.96	0.68	18.31	2	16.03	2.21	51	−0.09	0.03	0.02	2
Collinder 359	MS	8.30		1.79	57.53^c	1	5.28	3.25	12	−0.66^d		0.08	1
Mamajek 4	MS	−28.09	2.19	0.98	6.95	5	−26.32	3.17	34	0.09	0.17	0.08	5
NGC 2243	RGB	59.32	0.57	0.23	7.36	6	59.63	1.06	4	−0.31	0.05	0.02	6	−0.43	0.04	16	1
NGC 2516	MS	26.01	1.40	0.81	34.10^c	3	23.85	2.01	132	−0.26^d	0.05	0.03	3	0.06	0.05	13	1
NGC 2548	RGB	8.45	0.40	0.28	5.20	2	8.85	1.08	14	0.16	0.01	0.04	2
NGC 3680	MS	2.98		1.99	33.54^c	1	1.74	1.36	30	−0.26^d		0.07	1	−0.01	0.06	10	2
NGC 5460	MS	−5.16	0.31	0.22	23.79^c	2	−4.61	2.77	5	−0.32^d	0.15	0.11	2
Turner 5	MS	−2.83	0.09	0.07	11.77	2	−3.49	1.93	6	0.02	0.17	0.12	2

Notes.

^(a)

Mean of the individual values for those clusters with more than one star.

^(b)

From Soubiran et al. (2018).

^(c)

Values for clusters where ⟨v sin i⟩ > 20 km s⁻¹ are considered uncertain.

^(d)

[Fe/H] uncertain because ⟨v sin i⟩ > 20 km s⁻¹.

References. (1) Magrini et al. (2017); (2) Netopil et al. (2016)

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