CWNU 2336

0.26 UTI

0.26

C_N

0.2

C_dens

0.25

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 26

Stellar density (N₅₀/rad) 1.0 [N/pc²]

C3 classification DB

C_N 0.26 Poorly populated
C_dens 0.2 Very loose
C_C3 0.25 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

ℹ️

CWNU 2336 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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 metallicity 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 2336 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	204.699	-61.66	0.373	-8.095	-2.393	–
Hu & Soubiran	2025	204.646	-61.701	–	–	–	–
Hunt & Reffert	2024	204.749	-61.672	0.364	-8.094	-2.395	-38.98
Cavallo et al.	2024	204.646	-61.701	0.363	–	–	–
Hunt & Reffert	2023	204.749	-61.672	0.364	-8.094	-2.395	-38.98
He et al.	2023	204.589	-61.683	0.377	-8.106	-2.387	-75.78

💡 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–	2.4	1.91	1.33	525	0.005	171	–	–
Hu & Soubiran	2025	–	–	–	–	-0.410⁽⁵⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	171⁽¹⁾	–	–
Cavallo et al.	2024	2.34	1.71	–	525	0.420	–	–	–
Hunt & Reffert	2023	2.47	1.91	1.33	209	–	–	–	–
He et al.	2023	2.40	1.95	–	631	–	–	–	–

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

Visualization

ℹ️

1 2