CWNU 2112

0.18 UTI

0.0

C_N

0.16

C_dens

0.12

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 0.8 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.12 Very low 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 2112 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, below 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.

Data

🔍 Search references for CWNU 2112 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–	57.279	50.264	0.599	-1.014	-2.634	-16.391
Zhang et al.	2024	57.323	50.238	–	–	–	–
Hunt & Reffert	2024	57.323	50.238	0.6	-0.988	-2.654	-29.592
Cavallo et al.	2024	57.248	50.267	0.599	–	–	–
Hunt & Reffert	2023	57.323	50.238	0.6	-0.988	-2.654	-29.592
He et al.	2023	57.391	50.214	0.6	-1.004	-2.611	-29.58

💡 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–	1.61	2.6	1.44	158	0.036	107	–	–
Zhang et al.	2024	–	–	–	–	0.092⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	107⁽¹⁾	–	–
Cavallo et al.	2024	2.06	2.71	–	112	-0.020	–	–	–
Hunt & Reffert	2023	1.61	2.15	1.44	414	–	–	–	–
He et al.	2023	1.55	2.60	–	158	–	–	–	–

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

Visualization

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