CWNU 329

0.05 UTI

0.6

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.1

C_dup

C3 classification AB

Number of members (P>50%) 70

Radius (P>50% members) 4.0 [arcmin]

C_N 0.6 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High 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 329 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate 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 Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWNU 329 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	–	107.203	-9.431	0.344	-0.481	-0.369	27.936
He et al.	2022	107.295	-9.493	0.35	-0.5	-0.36	–

💡 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	2.51	1.50	–	398	-0.236	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1173	90.0	107.19	-9.42	0.34	-0.47	-0.38	27.94	0.68
UBC 1358	80.0	107.18	-9.42	0.34	-0.46	-0.39	13.04	0.0

💡 Note: The % column shows the percentage of members that CWNU 329 shares with each listed object.

Visualization

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