CWWDL 5708

0.08 UTI

0.25

C_N

0.11

C_dens

0.12

C_C3

0.0

C_lit

0.84

C_dup

C3 classification DC

Number of members (P>50%) 25

Radius (P>50% members) 7.3 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.11 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.84 Very likely unique

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

Overview

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CWWDL 5708 is a poorly populated, 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 near-solar metallicity, 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=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 5708 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	–	280.691	-6.294	0.314	0.268	-1.003	23.038
Chi et al.	2023	280.719	-6.266	0.298	0.274	-0.989	17.559

💡 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	–	–	–	58	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 104	16.0	280.71	-6.25	0.33	0.47	-0.8	14.46	0.72

💡 Note: The % column shows the percentage of members that CWWDL 5708 shares with each listed object.

Visualization

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