CWNU 2467

0.28 UTI

0.43

C_N

0.07

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 43

Core radius and density 2.1 [pc], 0.4 [pc^-2]

C3 classification AB

C_N 0.43 Poorly populated
C_dens 0.07 Very loose
C_C3 0.75 High quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 2467 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.98 (50th percentile), true positive (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.98 (50th percentile), true positive (human-assigned).

Data

🔍 Search references for CWNU 2467 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–	308.102	48.224	0.37	-2.406	-4.736	–
Hunt & Reffert	2024	308.07	48.223	0.366	-2.417	-4.729	–
Cavallo et al.	2024	308.098	48.231	0.367	–	–	–
Hunt & Reffert	2023	308.07	48.223	0.366	-2.417	-4.729	–
He et al.	2023	308.085	48.186	0.371	-2.406	-4.729	-26.7

💡 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–	2.52	1.47	2.54	138	0.290	266	–	–
Hunt & Reffert	2024	2.52	1.34	2.54	138	–	266⁽¹⁾	–	–
Cavallo et al.	2024	2.92	1.81	–	44	0.290	–	–	–
Hunt & Reffert	2023	2.52	1.34	2.54	138	–	–	–	–
He et al.	2023	2.45	1.60	–	447	–	–	–	–

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

Visualization

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