CWNU 485

0.01 UTI

0.31

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.03

C_dup

N₅₀ (P>50% members) 31

Stellar density (N₅₀/rad) 25.1 [N/pc²]

C3 classification CB

C_N 0.31 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 485 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as an extremely metal-poor, old cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Moderate extinction Extremely metal-poor Old

Data

🔍 Search references for CWNU 485 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–	198.849	-61.597	0.576	-6.772	-1.697	–
He et al.	2022	198.843	-61.603	0.57	-6.77	-1.69	–

💡 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–	1.38	2.22	–	1585	-2.028	–	–	–
He et al.	2022	1.38	2.22	–	1585	-2.028	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0596	96.8	198.85	-61.59	0.57	-6.77	-1.7	–	0.44

💡 Note: The % column shows the percentage of members that CWNU 485 shares with each listed object.

Visualization

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