CWWDL 14541

0.17 UTI

0.0

C_N

0.24

C_dens

0.62

C_C3

0.0

C_lit

0.96

C_dup

C3 classification CA

Number of members (P>50%) 21

Radius (P>50% members) 39.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.24 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

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

Overview

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CWWDL 14541 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, below 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 is 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=0.96) 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 14541 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	–	83.575	-3.184	2.764	1.458	-1.655	15.037
Chi et al.	2023	83.525	-3.783	2.745	1.326	-1.724	13.339

💡 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	–	–	–	0	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 17 a	4.0	83.45	-1.71	2.76	1.61	-1.22	17.6	0.55

💡 Note: The % column shows the percentage of members that CWWDL 14541 shares with each listed object.

Visualization

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