CWNU 3359

0.29 UTI

0.78

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.61

C_dup

C3 classification AC

Number of members (P>50%) 168

Radius (P>50% members) 1.7 [arcmin]

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.61 Likely unique

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

Overview

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CWNU 3359 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very distant High extinction Old

Data

🔍 Search references for CWNU 3359 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	–	300.529	33.91	0.137	-2.324	-4.883	8.376
He et al.	2023	300.529	33.911	0.084	-2.34	-4.877	10.03

💡 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	6.03	4.20	–	1259	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0188	39.3	300.53	33.91	0.14	-2.34	-4.88	10.03	0.61

💡 Note: The % column shows the percentage of members that CWNU 3359 shares with each listed object.

Visualization

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