CWWDL 14193

0.16 UTI

0.0

C_N

0.23

C_dens

0.75

C_C3

0.0

C_lit

0.84

C_dup

C3 classification AB

Number of members (P>50%) 19

Radius (P>50% members) 8.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.23 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.84 Very likely unique

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

Overview

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CWWDL 14193 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a metal-poor, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a 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=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Metal-poor Very young

Data

🔍 Search references for CWWDL 14193 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	–	253.36	-41.474	0.632	-0.662	-1.937	-15.256
Chi et al.	2023	253.422	-41.491	0.662	-0.648	-1.937	-30.8

💡 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
Chi et al.	2023	–	–	–	2	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 6231	16.0	253.56	-41.83	0.6	-0.58	-2.18	-27.67	1.0
UBC 672	4.0	253.28	-41.61	0.57	-0.64	-2.02	-26.66	0.1

💡 Note: The % column shows the percentage of members that CWWDL 14193 shares with each listed object.

Visualization

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