CWNU 374

0.04 UTI

0.4

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.1

C_dup

C3 classification BB

Number of members (P>50%) 40

Radius (P>50% members) 3.0 [arcmin]

C_N 0.4 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.1 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 374 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 low extinction. It is catalogued as a near-solar metallicity, 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 Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWNU 374 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	–	110.184	-17.877	0.355	-1.011	1.354	46.98
He et al.	2022	110.19	-17.873	0.35	-1.01	1.35	–

💡 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.	2022	2.57	0.90	–	316	0.457	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1372	90.0	110.18	-17.88	0.35	-1.01	1.35	46.98	0.54
CWWDL 633	67.5	110.18	-17.87	0.36	-1.02	1.34	–	0.04

💡 Note: The % column shows the percentage of members that CWNU 374 shares with each listed object.

Visualization

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