CWWDL 8368

0.02 UTI

0.0

C_N

0.2

C_dens

0.5

C_C3

0.0

C_lit

0.16

C_dup

N_m (P>50%) 19

Core radius and density 1.6 [pc], 1.0 [pc^-2]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.2 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 8368 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near 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 8368 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–	3.263	62.477	0.313	-2.088	-0.947	–
Chi et al.	2023	3.153	62.467	0.326	-2.125	-0.941	–

💡 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–	–	–	–	141	-0.880	–	–	–
Chi et al.	2023	–	–	–	141	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Casado 15	84.0	3.26	62.47	0.31	-2.08	-0.92	-102.11	0.23
OC 0220	72.0	3.29	62.47	0.31	-2.04	-0.93	–	0.02

💡 Note: The % column shows the percentage of members that CWWDL 8368 shares with each listed object.

Visualization

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