CWNU 3722

0.13 UTI

0.0

C_N

0.1

C_dens

0.62

C_C3

0.0

C_lit

0.92

C_dup

C3 classification AC

Number of members (P>50%) 20

Radius (P>50% members) 9.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.92 Very likely unique

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

Overview

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CWNU 3722 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small 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=0.92) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low extinction Very young

Data

🔍 Search references for CWNU 3722 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	–	204.137	-63.645	0.454	-3.617	-1.708	6.702
He et al.	2023	204.207	-63.609	0.454	-3.573	-1.677	–

💡 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	2.09	0.05	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 3381	8.0	203.68	-63.33	0.47	-3.82	-1.63	–	0.35

💡 Note: The % column shows the percentage of members that CWNU 3722 shares with each listed object.

Visualization

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