CWNU 185

0.00 UTI

0.29

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 29

Stellar density (N₅₀/rad) 6.0 [N/pc²]

C3 classification CA

C_N 0.29 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 185 is a poorly populated, very dense object of intermediate 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, very young 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 High extinction Metal-rich Very young

Data

🔍 Search references for CWNU 185 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–	134.936	-45.806	0.474	-4.858	4.811	-150.206
He et al.	2022	134.935	-45.815	0.47	-4.87	4.79	–

💡 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	4.08	–	6	0.916	–	–	–
He et al.	2022	2.95	4.08	–	6	0.916	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1451	100.0	134.93	-45.82	0.48	-4.86	4.8	11.79	0.65

💡 Note: The % column shows the percentage of members that CWNU 185 shares with each listed object.

Visualization

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