CWNU 2695

0.47 UTI

0.39

C_N

0.87

C_dens

0.5

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 39

Stellar density (N₅₀/rad) 4.4 [N/pc²]

C3 classification BB

C_N 0.39 Poorly populated
C_dens 0.87 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 2695 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate 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 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 2695 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–	176.16	-63.565	0.312	-7.154	-0.054	-24.551
Hu & Soubiran	2025	176.188	-63.572	–	–	–	–
Hunt & Reffert	2024	176.094	-63.55	0.306	-7.159	-0.049	-24.201
Cavallo et al.	2024	176.188	-63.572	0.311	–	–	–
Hunt & Reffert	2023	176.094	-63.55	0.306	-7.159	-0.049	-24.201
He et al.	2023	176.151	-63.563	0.312	-7.153	-0.053	-24.55

💡 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–	2.95	2.01	1.47	267	-0.090	275	–	–
Hu & Soubiran	2025	–	–	–	–	-0.250⁽⁵⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	275⁽¹⁾	–	–
Cavallo et al.	2024	2.24	1.54	–	575	0.070	–	–	–
Hunt & Reffert	2023	2.96	2.01	1.47	267	–	–	–	–
He et al.	2023	2.95	2.25	–	251	–	–	–	–

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

Visualization

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