CWNU 3125

0.01 UTI

0.64

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.02

C_dup

C3 classification AA

Number of members (P>50%) 79

Radius (P>50% members) 1.2 [arcmin]

C_N 0.64 Moderately 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 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3125 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large distance, well above the mid-plane, affected by moderate 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.

Very distant Moderate extinction Old

Data

🔍 Search references for CWNU 3125 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	–	328.871	63.938	0.118	-2.575	-1.429	-72.711
He et al.	2023	328.868	63.938	0.113	-2.577	-1.441	-80.5

💡 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]	Bfr	BSS
He et al.	2023	7.76	2.70	–	1259	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Berkeley 93	97.5	328.86	63.94	0.1	-2.59	-1.46	-72.71	0.81

💡 Note: The % column shows the percentage of members that CWNU 3125 shares with each listed object.

Visualization

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