The Radcliffe wave as traced by young open clusters - Stellar parameters, activity indicators, and abundances of solar-type members of eight young clusters

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Volume 691 (November 2024)

A&A, 691 (2024) A317

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Table 2

Stellar parameters of the components of SB2 systems derived with the code COMPO2.

Star	T_eff	err	log ɡ	err	RV	err	γ	$w_{4400}^{P}$ $w_{4400}^{\rm{P}}$	$w_{5500}^{P}$ $w_{5500}^{\rm{P}}$	$w_{6400}^{P}$ $w_{6400}^{\rm{P}}$	SpT	v sin i
	(K)	(K)	(dex)	(dex)	(km s⁻¹)		(km s⁻¹)					(km s⁻¹)
	[P/S]	[P/S]	[P/S]	[P/S]	[P/S]	[P/S]					[P/S]	[P/S]
Mel2O-Sll	6119/5172	75/240	4.02/3.92	0.14/0.62	31.74/–41.46	0.15/2.39	4.2 ± 1.2	0.91 ±0.02	0.89 ±0.02	0.90 ±0.03	F7IV/K1IV	8/8
Plei-S2	5674/5371	139/172	4.36/4.39	0.13/0.14	14.32/0.20	0.22/0.30	7.4 ± 0.2^(a)	0.56 ±0.03	0.55 ±0.03	0.53 ±0.03	G2V/G2V	4/3
ASCC19-S7	5376/4894	139/226	4.41/4.36	0.11/0.40	35.49/9.11	0.25/1.16	24.6 ± 0.5	0.87 ±0.02	0.83 ±0.02	0.79 ±0.04	G8V/K4V	7/7

Notes. ^(a)In very good agreement with the value of 7.434 km s⁻¹ reported by Torres et al. (2021).

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