CWNU 112

0.28 UTI

0.0

C_N

0.65

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 19

Stellar density (N₅₀/rad) 3.2 [N/pc²]

C3 classification DB

C_N 0.0 Sparse
C_dens 0.65 Moderately dense
C_C3 0.25 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 112 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

Relatively close High extinction Metal-rich Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 112 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–	302.077	33.945	0.432	-2.722	-5.593	80.456
Hunt & Reffert	2024	302.093	33.952	0.427	-2.741	-5.61	80.273
Cavallo et al.	2024	302.097	33.939	0.435	–	–	–
Hunt & Reffert	2023	302.093	33.952	0.427	-2.741	-5.61	80.273
He et al.	2022	302.061	33.968	0.4	-2.73	-5.55	-10.6

💡 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–	2.59	3.42	2.49	29	0.964	441	–	–
Hunt & Reffert	2024	–	–	–	–	–	441⁽¹⁾	–	–
Cavallo et al.	2024	2.59	3.15	–	60	0.960	–	–	–
Hunt & Reffert	2023	2.13	3.42	2.49	29	–	–	–	–
He et al.	2022	2.95	3.90	–	20	0.968	–	–	–

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

Visualization

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