CWWDL 14180

0.18 UTI

0.0

C_N

0.28

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 23

Core radius and density 1.4 [pc], 1.4 [pc^-2]

C3 classification AC

C_N 0.0 Sparse
C_dens 0.28 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14180 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14180 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–	119.341	-26.956	0.717	-2.24	3.344	38.206
Chi et al.	2023	119.343	-26.994	0.72	-2.308	3.385	47.731

💡 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–	–	–	–	2	-0.280	–	–	–
Chi et al.	2023	–	–	–	2	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1968	80.0	119.34	-26.97	0.72	-2.23	3.28	43.27	0.03

💡 Note: The % column shows the percentage of members that CWWDL 14180 shares with each listed object.

Visualization

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