CWNU 3355

0.21 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.41

C_dup

N₅₀ (P>50% members) 122

Stellar density (N₅₀/rad) 9.8 [N/pc²]

C3 classification AB

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.41 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3355 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Old

Data

🔍 Search references for CWNU 3355 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–	168.133	-59.698	0.272	-4.048	0.196	-12.931
He et al.	2023	168.135	-59.698	0.27	-4.05	0.205	-13.19

💡 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–	3.98	2.5	–	1000	–	–	–	–
He et al.	2023	3.98	2.50	–	1000	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2404	59.0	168.13	-59.7	0.27	-4.05	0.21	-13.19	0.57

💡 Note: The % column shows the percentage of members that CWNU 3355 shares with each listed object.

Visualization

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