CWWDL 10480

0.13 UTI

0.0

C_N

0.8

C_dens

1.0

C_C3

0.0

C_lit

0.36

C_dup

C3 classification AA

Number of members (P>50%) 19

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

C_N 0.0 Sparse
C_dens 0.8 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.36 Possibly duplicate

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

Overview

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CWWDL 10480 is a sparse, dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 10480 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	–	8.339	63.32	0.334	-2.818	-0.552	–
Chi et al.	2023	8.89	63.317	0.356	-2.797	-0.606	-48.974

💡 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	–	–	–	13	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 146	64.0	8.24	63.31	0.33	-2.85	-0.49	-99.85	0.94
FoF 1864	16.0	8.7	63.04	0.35	-2.91	-0.56	–	0.08

💡 Note: The % column shows the percentage of members that CWWDL 10480 shares with each listed object.

Visualization

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