CWWDL 3284

0.00 UTI

0.69

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 88

Radius (P>50% members) 4.5 [arcmin]

C_N 0.69 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

CWWDL 3284 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a metal-poor, young 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.

Metal-poor Young

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	83.767	15.718	0.701	0.254	-2.386	10.424
Chi et al.	2023	83.766	15.716	0.69	0.238	-2.378	20.118

💡 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	–	–	–	33	-0.880	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
COIN-Gaia 26	100.0	83.77	15.72	0.7	0.25	-2.4	10.42	0.77
LISC 0988	100.0	83.77	15.72	0.7	0.25	-2.39	10.42	0.04
UBC 75	98.9	83.77	15.72	0.7	0.26	-2.4	10.42	0.03

💡 Note: The % column shows the percentage of members that CWWDL 3284 shares with each listed object.

Visualization

💡 Note: How are the galactocentric plots generated? See FAQ.