CWWDL 11666

0.11 UTI

0.62

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.22

C_dup

N₅₀ (P>50% members) 73

Stellar density (N₅₀/rad) 6.0 [N/pc²]

C3 classification AA

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.22 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 11666 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 11666 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–	318.412	50.134	0.6	-2.912	-4.101	-8.217
Chi et al.	2023	318.356	50.135	0.593	-2.901	-4.108	-10.107

💡 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–	–	–	–	123	-0.880	–	–	–
Chi et al.	2023	–	–	–	123	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 155	78.1	318.43	50.13	0.6	-2.92	-4.09	-13.71	0.64

💡 Note: The % column shows the percentage of members that CWWDL 11666 shares with each listed object.

Visualization

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