CWNU 119

0.18 UTI

0.0

C_N

0.29

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 1.5 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.29 Loose
C_C3 0.12 Very low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 119 is a sparse, loose object of very low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Moderate extinction Low mass Near-solar metallicity Young

Palma et al. (2025)
Part of multiple system G104, along with King_6 and HSC_1146.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 119 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	47.433	57.926	1.36	0.915	-5.061	-6.872
Hunt & Reffert	2024	47.45	57.934	1.354	0.886	-5.034	-4.376
Cavallo et al.	2024	47.154	57.952	1.355	–	–	–
Hunt & Reffert	2023	47.45	57.934	1.354	0.886	-5.034	-4.376
He et al.	2022	47.456	57.938	1.36	0.91	-5.06	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	0.71	1.95	0.98	57	0.364	43	–	–
Hunt & Reffert	2024	–	–	–	–	–	43⁽¹⁾	–	–
Cavallo et al.	2024	0.82	1.93	–	32	0.560	–	–	–
Hunt & Reffert	2023	0.70	1.95	0.98	57	–	–	–	–
He et al.	2022	0.71	1.98	–	158	0.169	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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