CWWDL 10668

0.03 UTI

0.0

C_N

0.03

C_dens

0.25

C_C3

0.0

C_lit

0.6

C_dup

C3 classification CC

Number of members (P>50%) 16

Radius (P>50% members) 13.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.6 Likely unique

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

Overview

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CWWDL 10668 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above 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 likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 10668 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	–	39.852	60.769	0.391	-0.557	-0.341	-41.751
Chi et al.	2023	39.654	60.771	0.391	-0.559	-0.336	-48.265

💡 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	–	–	–	23	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 420	40.0	40.37	60.84	0.43	-0.65	-0.21	-61.21	0.47
CWWDL 2624	28.0	40.35	60.76	0.41	-0.5	-0.3	-81.55	0.04
Berkeley 65	12.0	39.77	60.4	0.45	-0.72	-0.4	-60.43	0.82

💡 Note: The % column shows the percentage of members that CWWDL 10668 shares with each listed object.

Visualization

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