CWWDL 4703

0.08 UTI

0.0

C_N

0.05

C_dens

0.5

C_C3

0.0

C_lit

0.76

C_dup

C3 classification BB

Number of members (P>50%) 15

Radius (P>50% members) 9.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.76 Very likely unique

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

Overview

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CWWDL 4703 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 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=0.76) 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 4703 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	–	106.419	-9.125	0.351	-1.09	0.892	–
Chi et al.	2023	106.412	-9.139	0.346	-1.06	0.829	–

💡 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	–	–	–	1	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 218	24.0	106.52	-9.18	0.35	-1.18	0.89	–	0.16
OC 0375	8.0	106.76	-9.17	0.37	-1.17	0.91	–	0.27
Theia 1774	4.0	106.74	-9.17	0.37	-1.17	0.91	–	0.01

💡 Note: The % column shows the percentage of members that CWWDL 4703 shares with each listed object.

Visualization

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