CWNU 130

0.03 UTI

0.32

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.09

C_dup

N₅₀ (P>50% members) 32

Stellar density (N₅₀/rad) 5.3 [N/pc²]

C3 classification BB

C_N 0.32 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.09 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 130 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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 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 Metal-rich Intermediate age

Data

🔍 Search references for CWNU 130 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–	101.167	-2.787	0.46	-0.784	0.234	73.934
He et al.	2022	101.198	-2.78	0.46	-0.79	0.24	54.4

💡 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	1.38	–	158	0.805	–	–	–
He et al.	2022	2.75	1.38	–	158	0.805	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1345	90.6	101.17	-2.79	0.46	-0.78	0.23	73.93	0.51

💡 Note: The % column shows the percentage of members that CWNU 130 shares with each listed object.

Visualization

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