CWWDL 2585

0.25 UTI

0.5

C_N

0.19

C_dens

0.62

C_C3

0.0

C_lit

0.96

C_dup

C3 classification AC

Number of members (P>50%) 51

Radius (P>50% members) 8.4 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.19 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

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

Overview

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CWWDL 2585 is a moderately populated, very 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, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small 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 2585 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	–	356.003	62.661	0.333	-3.678	-1.47	-65.428
Chi et al.	2023	356.071	62.679	0.345	-3.727	-1.556	-51.548

💡 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	–	–	–	2	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 219	3.9	356.06	62.67	0.37	-3.84	-1.92	–	0.02
UBC 1189	2.0	356.06	62.67	0.37	-3.84	-1.92	–	0.53

💡 Note: The % column shows the percentage of members that CWWDL 2585 shares with each listed object.

Visualization

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