CWWDL 2285

0.04 UTI

0.81

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.07

C_dup

N₅₀ (P>50% members) 255

Stellar density (N₅₀/rad) 50.2 [N/pc²]

C3 classification AA

C_N 0.81 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.07 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 2285 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 2285 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	99999–	251.898	-44.539	0.4	-1.603	-3.146	-19.895
Chi et al.	2023	251.905	-44.541	0.413	-1.623	-3.16	-19.787

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	107	-0.280	–	–	–
Chi et al.	2023	–	–	–	107	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 321	92.9	251.89	-44.54	0.39	-1.59	-3.14	-19.86	0.7

💡 Note: The % column shows the percentage of members that CWWDL 2285 shares with each listed object.

Visualization

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