CWNU 104

0.02 UTI

0.28

C_N

0.62

C_dens

0.25

C_C3

0.0

C_lit

0.11

C_dup

N₅₀ (P>50% members) 28

Stellar density (N₅₀/rad) 3.1 [N/pc²]

C3 classification CC

C_N 0.28 Poorly populated
C_dens 0.62 Moderately dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.11 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 104 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is 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 Metal-rich Intermediate age

Data

🔍 Search references for CWNU 104 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–	95.994	20.513	0.445	0.136	-1.349	42.298
He et al.	2022	96.001	20.518	0.45	0.14	-1.35	31.8

💡 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–	2.75	1.62	–	316	0.968	–	–	–
He et al.	2022	2.75	1.62	–	316	0.968	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1611	89.3	95.99	20.51	0.45	0.14	-1.34	42.3	0.41

💡 Note: The % column shows the percentage of members that CWNU 104 shares with each listed object.

Visualization

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