CWWDL 2584

0.27 UTI

0.57

C_N

0.34

C_dens

0.75

C_C3

0.0

C_lit

0.8

C_dup

C3 classification AB

Number of members (P>50%) 65

Radius (P>50% members) 6.6 [arcmin]

C_N 0.57 Moderately populated
C_dens 0.34 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.8 Very likely unique

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

Overview

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CWWDL 2584 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near 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 very likely a unique object, which shares a 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 2584 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	–	356.444	62.135	0.312	-3.589	-1.564	–
Chi et al.	2023	356.348	62.164	0.31	-3.539	-1.561	-57.058

💡 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	–	–	–	1	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Stock 17	20.0	355.97	62.16	0.32	-3.7	-1.56	–	0.64

💡 Note: The % column shows the percentage of members that CWWDL 2584 shares with each listed object.

Visualization

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