CWWDL 10380

0.04 UTI

0.0

C_N

0.08

C_dens

0.12

C_C3

0.0

C_lit

0.88

C_dup

C3 classification DC

Number of members (P>50%) 17

Radius (P>50% members) 5.3 [arcmin]

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.88 Very likely unique

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

Overview

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CWWDL 10380 is a sparse, very loose object of very low 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.

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=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 10380 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	–	334.246	56.753	0.231	-3.329	-2.885	–
Chi et al.	2023	334.224	56.753	0.237	-3.388	-2.831	-77.715

💡 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	–	–	–	200	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0356	12.0	334.68	56.77	0.24	-3.18	-2.76	–	0.03

💡 Note: The % column shows the percentage of members that CWWDL 10380 shares with each listed object.

Visualization

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