Tracing the W3/W4/W5 and Perseus complex dynamical evolution with star clusters

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Table 4

Six-dimensional coordinates of the star clusters within the Perseus complex analyzed in this work.

Cluster	α₀ (°)	δ₀ (°)	〈d〉 (pc)	〈μ_α*〉 (mas yr⁻¹)	〈μ_δ〉 (mas yr⁻¹)	υ_LOS (km s⁻¹)	N_LOS	source
Berkeley 65	39.769	60.403	2013 $_{- 18}^{+ 19}$ $^{+19}_{-18}$	$- {0.688}_{- 0.014}^{+ 0.014}$ ${-}0.688^{+0.014}_{-0.014}$	$- {0.423}_{- 0.014}^{+ 0.013}$ ${-}0.423^{+0.013}_{-0.014}$	−60.4 ± 7.0	1	(1)
IC 1805	38.198	61.469	1982 $_{- 9}^{+ 10}$ $^{+10}_{-9}$	$- {0.741}_{- 0.015}^{+ 0.015}$ ${-}0.741^{+0.015}_{-0.015}$	$- {0.735}_{- 0.015}^{+ 0.015}$ ${-}0.735^{+0.015}_{-0.015}$	−43.8 ± 3.0	18	(0)
IC 1848	42.816	60.412	2004 $_{- 9}^{+ 9}$ $^{+9}_{-9}$	$- {0.405}_{- 0.014}^{+ 0.015}$ ${-}0.405^{+0.015}_{-0.014}$	$- {0.431}_{- 0.011}^{+ 0.011}$ ${-}0.431^{+0.011}_{-0.011}$	−37.0 ± 3.3	16	(0)
SAI 24	44.732	60.577	1989 $_{- 9}^{+ 10}$ $^{+10}_{-9}$	$- {0.257}_{- 0.019}^{+ 0.018}$ ${-}0.257^{+0.018}_{-0.019}$	${0.068}_{- 0.012}^{+ 0.012}$ $0.068^{+0.012}_{-0.012}$	−48.5 ± 5.4	7	(1)
UBC 420	40.172	60.862	2106 $_{- 7}^{+ 7}$ $^{+7}_{-7}$	$- {0.599}_{- 0.017}^{+ 0.017}$ ${-}0.599^{+0.017}_{-0.017}$	$- {0.298}_{- 0.008}^{+ 0.008}$ ${-}0.298^{+0.008}_{-0.008}$	–	–	–
NGC 884	35.513	57.148	2220 $_{- 12}^{+ 15}$ $^{+15}_{-12}$	$- {0.620}_{- 0.010}^{+ 0.011}$ ${-}0.620^{+0.011}_{-0.010}$	$- {1.153}_{- 0.014}^{+ 0.013}$ ${-}1.153^{+0.013}_{-0.014}$	−33.7 ± 4.0	5	(0)
NGC 869	34.736	57.130	2217 $_{- 11}^{+ 12}$ $^{+12}_{-11}$	$- {0.651}_{- 0.009}^{+ 0.010}$ ${-}0.651^{+0.010}_{-0.009}$	$- {1.161}_{- 0.012}^{+ 0.011}$ ${-}1.161^{+0.011}_{-0.012}$	−67.6 ± 10.4	6	(1)
NGC 957	38.348	57.559	2155 $_{- 20}^{+ 19}$ $^{+19}_{-20}$	$- {0.303}_{- 0.014}^{+ 0.016}$ ${-}0.303^{+0.016}_{-0.014}$	$- {1.132}_{- 0.012}^{+ 0.012}$ ${-}1.132^{+0.012}_{-0.012}$	−37.5 ± 5.5	2	(1)
Basel 10	34.879	58.291	2002 $_{- 19}^{+ 19}$ $^{+19}_{-19}$	$- {0.422}_{- 0.015}^{+ 0.014}$ ${-}0.422^{+0.014}_{-0.015}$	$- {0.839}_{- 0.013}^{+ 0.012}$ ${-}0.839^{+0.012}_{-0.013}$	–	–	–
NGC 654	26.004	61.883	2699 $_{- 19}^{+ 20}$ $^{+20}_{-19}$	$- {1.140}_{- 0.006}^{+ 0.007}$ ${-}1.140^{+0.007}_{-0.006}$	$- {0.336}_{- 0.007}^{+ 0.006}$ ${-}0.336^{+0.006}_{-0.007}$	−20.6 ± 8.1	3	(1)
NGC 663	26.574	61.195	2610 $_{- 11}^{+ 13}$ $^{+13}_{-11}$	$- {1.140}_{- 0.004}^{+ 0.004}$ ${-}1.140^{+0.004}_{-0.004}$	$- {0.326}_{- 0.004}^{+ 0.004}$ ${-}0.326^{+0.004}_{-0.004}$	−24.9 ± 15.8	3	(1)
NGC 659	26.108	60.677	2843 $_{- 26}^{+ 23}$ $^{+23}_{-26}$	$- {0.831}_{- 0.004}^{+ 0.004}$ ${-}0.831^{+0.004}_{-0.004}$	$- {0.301}_{- 0.004}^{+ 0.005}$ ${-}0.301^{+0.005}_{-0.004}$	−48.2 ± 13.0	2	(1)
NGC 581	23.339	60.664	2468 $_{- 15}^{+ 17}$ $^{+17}_{-15}$	$- {1.387}_{- 0.006}^{+ 0.006}$ ${-}1.387^{+0.006}_{-0.006}$	$- {0.597}_{- 0.005}^{+ 0.005}$ ${-}0.597^{+0.005}_{-0.005}$	−38.1 ± 4.4	2	(1)
Berkeley 6	27.801	61.059	2702 $_{- 27}^{+ 31}$ $^{+31}_{-27}$	$- {0.900}_{- 0.009}^{+ 0.009}$ ${-}0.900^{+0.009}_{-0.009}$	$- {0.527}_{- 0.009}^{+ 0.009}$ ${-}0.527^{+0.009}_{-0.009}$	−88.9 ± 5.9	2	(1)
Berkeley 7	28.545	62.367	2597 $_{- 29}^{+ 27}$ $^{+27}_{-29}$	$- {0.980}_{- 0.006}^{+ 0.006}$ ${-}0.980^{+0.006}_{-0.006}$	$- {0.220}_{- 0.007}^{+ 0.007}$ ${-}0.220^{+0.007}_{-0.007}$	−48.4 ± 5.1	1	(0)
Czernik 6	30.539	62.839	2653 $_{- 30}^{+ 29}$ $^{+29}_{-30}$	$- {1.184}_{- 0.007}^{+ 0.008}$ ${-}1.184^{+0.008}_{-0.007}$	$- {0.186}_{- 0.013}^{+ 0.011}$ ${-}0.186^{+0.011}_{-0.013}$	−56.26 ± 0.03	1	(0)
Riddle 4	31.868	60.258	2588 $_{- 29}^{+ 26}$ $^{+26}_{-29}$	$- {0.808}_{- 0.010}^{+ 0.009}$ ${-}0.808^{+0.009}_{-0.010}$	$- {0.503}_{- 0.012}^{+ 0.011}$ ${-}0.503^{+0.011}_{-0.012}$	−25.3 ± 20.3	3	(1)
NGC 637	25.775	64.041	2524 $_{- 17}^{+ 18}$ $^{+18}_{-17}$	$- {1.259}_{- 0.007}^{+ 0.006}$ ${-}1.259^{+0.006}_{-0.007}$	$- {0.027}_{- 0.006}^{+ 0.006}$ ${-}0.027^{+0.006}_{-0.006}$	–	–	–

Notes. Cluster name, center equatorial coordinates, distance from the Sun, PM components, LOS velocity, number of stars used in v_LOS calculation, and source catalog for the LOS velocity: (0) for Tarricq et al. (2021), and (1) for Hunt & Reffert (2023).

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