CWWDL 10477

0.12 UTI

0.0

C_N

0.44

C_dens

0.5

C_C3

0.0

C_lit

0.64

C_dup

C3 classification BB

Number of members (P>50%) 20

Radius (P>50% members) 2.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.44 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

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

Overview

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CWWDL 10477 is a sparse, loose object of intermediate 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 small 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 10477 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	–	12.921	63.822	0.241	-1.762	-0.303	-80.39
Chi et al.	2023	12.803	63.825	0.243	-1.848	-0.274	-29.709

💡 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	–	–	–	44	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 412	36.0	12.93	63.82	0.23	-1.62	-0.28	–	0.55
CWWDL 10490	12.0	13.32	63.7	0.23	-1.86	-0.33	-87.47	0.04

💡 Note: The % column shows the percentage of members that CWWDL 10477 shares with each listed object.

Visualization

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