CWWDL 14536

0.24 UTI

0.4

C_N

0.15

C_dens

1.0

C_C3

0.0

C_lit

0.78

C_dup

N_m (P>50%) 40

Core radius and density 1.6 [pc], 0.7 [pc^-2]

C3 classification AA

C_N 0.4 Poorly populated
C_dens 0.15 Very loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.78 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14536 is a poorly populated, very loose object of very high 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 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=0.78) 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 14536 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–	79.781	-1.288	2.733	1.525	-0.49	17.247
Chi et al.	2023	79.729	-1.136	2.766	1.529	-0.532	16.744

💡 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–	–	–	–	6	0.420	–	–	–
Chi et al.	2023	–	–	–	6	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWL 3512	22.5	80.71	-1.29	2.92	1.28	-0.36	16.24	0.38

💡 Note: The % column shows the percentage of members that CWWDL 14536 shares with each listed object.

Visualization

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