CWNU 71

0.12 UTI

0.36

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.28

C_dup

N₅₀ (P>50% members) 36

Stellar density (N₅₀/rad) 15.2 [N/pc²]

C3 classification AB

C_N 0.36 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 71 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Metal-rich Very young

Data

🔍 Search references for CWNU 71 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–	17.853	57.561	0.416	-2.158	-1.294	-53.585
He et al.	2022	17.855	57.575	0.42	-2.19	-1.31	–

💡 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–	3.09	1.26	–	6	0.916	–	–	–
He et al.	2022	3.09	1.26	–	6	0.916	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0233	72.2	17.84	57.56	0.41	-2.15	-1.31	-47.6	0.5

💡 Note: The % column shows the percentage of members that CWNU 71 shares with each listed object.

Visualization

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