CWNU 3190

0.01 UTI

0.81

C_N

0.62

C_dens

0.75

C_C3

0.0

C_lit

0.02

C_dup

N_m (P>50%) 251

Core radius and density 2.9 [pc], 3.1 [pc^-2]

C3 classification AB

C_N 0.81 Rich
C_dens 0.62 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3190 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It was recently reported 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.

Note: This object contains blue stragglers according to at least one source.

Very distant High extinction Old Contains BSS

Data

🔍 Search references for CWNU 3190 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–	308.639	49.948	0.201	-3.442	-4.977	-72.582
Cui et al.	2025	308.631	49.944	0.2	-3.44	-4.98	–
He et al.	2023	308.637	49.944	0.198	-3.436	-4.984	-72.87

💡 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–	5.37	4.05	–	1682	–	–	–	2
Cui et al.	2025	–	3.95	–	1778	–	–	–	2⁽¹⁾
He et al.	2023	5.37	4.15	–	1585	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0276	97.6	308.63	49.95	0.21	-3.44	-4.98	-72.34	0.51

💡 Note: The % column shows the percentage of members that CWNU 3190 shares with each listed object.

Visualization

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