CWNU 533

(OCSN 110)

0.00 UTI

0.0

C_N

0.04

C_dens

0.38

C_C3

0.03

C_lit

0.0

C_dup

N_m (P>50%) 22

Core radius and density 3.9 [pc], 0.2 [pc^-2]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.38 Low quality
C_lit 0.03 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 533 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied 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.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 533 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–	357.124	55.144	2.271	5.253	-4.463	-13.415
Qin et al.	2023	356.19	54.99	2.28	5.28	-4.47	-13.41
He et al.	2022	356.947	54.996	2.362	5.246	-4.441	–
He et al.	2022	358.114	55.399	2.24	5.29	-4.55	-12.5

💡 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]	B_frac	BSS
UCC	99999–	0.61	0.88	–	79	0.265	–	–	–
Qin et al.	2023	0.63	0.88	–	79	–	–	–	–
He et al.	2022	–	0.80	–	79	–	–	–	–
He et al.	2022	0.59	1.20	–	50	0.265	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 391	100.0	356.34	55.15	2.25	5.13	-4.41	-13.09	0.36

💡 Note: The % column shows the percentage of members that CWNU 533 shares with each listed object.

Visualization

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