A multi-frequency, multi-epoch radio continuum study of the Quintuplet cluster with the Very Large Array

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Table 1

Proper motions and cluster membership probability of the Quintuplet sources.

ID	µ_α cos δ	µ_δ	p_cluster
qF257	−1.12 ± 0.08	−2.52 ± 0.09	0.64
qF241	−0.98 ± 0.09	−2.36 ± 0.09	0.93
qF240	−0.84 ± 0.07	−2.37 ± 0.09	0.90
qF320	−1.13 ± 0.10	−2.39 ± 0.09	0.84
Muno7679	−0.82 ± 0.16	−2.50 ± 0.18	0.78
Dong66	−0.93 ± 0.06	−2.61 ± 0.08	0.48
qF256	−0.74 ± 0.10	−2.48 ± 0.12	0.70
qF270S	−1.21 ± 0.09	−2.41 ± 0.09	0.63
qF235S	−0.88 ± 0.07	−2.24 ± 0.08	0.94
qF307A	−0.99 ± 0.12	−2.46 ± 0.12	0.86
qF344	−0.85 ± 0.15	−2.47 ± 0.17	0.82
qF235N	−0.93 ± 0.07	−2.27 ± 0.08	0.94
qF353E	−0.96 ± 0.10	−2.43 ± 0.10	0.89
qF381	−1.07 ± 0.13	−2.55 ± 0.14	0.71
qF278	−1.05 ± 0.08	−2.30 ± 0.09	0.92
qF309	−0.82 ± 0.16	−2.34 ± 0.17	0.86
LHO100	−0.96 ± 0.09	−2.48 ± 0.09	0.85
qF274	−1.04 ± 0.14	−2.42 ± 0.15	0.86
Hos332	−1.14 ± 0.13	−2.29 ± 0.14	0.84
LHO076	−1.02 ± 0.07	−2.27 ± 0.07	0.94
WR102ca	−1.14 ± 0.07	−2.20 ± 0.06	0.84
LHO090	−1.09 ± 0.08	−2.20 ± 0.08	0.89
qF243	−1.24 ± 0.08	−2.45 ± 0.07	0.46
Hos18	−1.11 ± 0.08	−2.32 ± 0.07	0.89
qF250	−0.75 ± 0.30	−2.66 ± 0.33	0.56
LHO001	−0.90 ± 0.08	−2.44 ± 0.11	0.89
qF258	−1.01 ± 0.08	−2.40 ± 0.07	0.92
qF358	−0.91 ± 0.17	−2.58 ± 0.18	0.71
qF251	−1.20 ± 0.08	−2.40 ± 0.08	0.70
Dong72	−0.88 ± 0.10	−2.50 ± 0.12	0.82
Hos21	−0.98 ± 0.07	−2.35 ± 0.06	0.94
Hos95	−0.73 ± 0.13	−2.64 ± 0.15	0.41
qF406	−1.47 ± 0.16	−2.32 ± 0.17	0.18
qF276	−0.88 ± 0.08	−2.56 ± 0.07	0.61
LHO029	−0.97 ± 0.08	−2.39 ± 0.08	0.92
qG29^(a)	−2.30 ± 0.11	−3.59 ± 0.08	0.00

Notes. Proper motion and cluster membership probability values from Hosek et al. (2022). All proper motion units in milli-arcseconds per year (mas yr⁻¹). The counterparts of qF362, qF211, qF231, qCG1, qCG2, and qF134 were not found in Hosek et al. (2022) catalogue within 0.″2 of our point sources.^(a) ID from Gallego-Calvente et al. (2022).

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