CWNU 460

0.49 UTI

0.34

C_N

1.0

C_dens

0.5

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 34

Stellar density (N₅₀/rad) 5.1 [N/pc²]

C3 classification DA

C_N 0.34 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.3 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 460 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close 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 and metallicity parameters (see Parameters). It is poorly studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 460 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–	308.387	43.745	0.886	0.253	-1.626	-18.909
Zhang et al.	2024	308.409	43.745	–	–	–	–
Hunt & Reffert	2024	308.409	43.745	0.852	0.292	-1.637	-20.769
Cavallo et al.	2024	308.393	43.73	0.87	–	–	–
Hunt & Reffert	2023	308.409	43.745	0.852	0.292	-1.637	-20.769
He et al.	2022	308.397	43.75	0.88	0.28	-1.61	-53.1

💡 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–	1.1	2.49	2.32	234	-0.148	158	–	–
Zhang et al.	2024	–	–	–	–	-0.148⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	158⁽¹⁾	–	–
Cavallo et al.	2024	1.19	2.63	–	234	0.020	–	–	–
Hunt & Reffert	2023	1.10	2.49	2.32	95	–	–	–	–
He et al.	2022	0.83	2.46	–	794	-0.642	–	–	–

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

Visualization

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