CWNU 3094

0.01 UTI

0.49

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.02

C_dup

N₅₀ (P>50% members) 49

Stellar density (N₅₀/rad) 6.1 [N/pc²]

C3 classification AA

C_N 0.49 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very 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 3094 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as an intermediate-age 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.

Relatively close Low extinction Intermediate age

Data

🔍 Search references for CWNU 3094 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–	272.403	-24.541	0.818	0.384	-2.404	-14.889
He et al.	2023	272.425	-24.541	0.816	0.386	-2.399	-21.7

💡 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–	1.23	1.0	–	251	–	–	–	–
He et al.	2023	1.23	1.00	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
ESO 521 38	98.0	272.4	-24.54	0.82	0.38	-2.41	-14.89	0.78

💡 Note: The % column shows the percentage of members that CWNU 3094 shares with each listed object.

Visualization

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