CWWDL 14569

0.29 UTI

0.68

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.54

C_dup

C3 classification AA

Number of members (P>50%) 85

Radius (P>50% members) 22.0 [arcmin]

C_N 0.68 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.54 Likely unique

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

Overview

ℹ️

CWWDL 14569 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below 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 likely a unique object, which shares a moderate 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 14569 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	82.848	12.097	2.508	0.761	-0.802	17.386
Chi et al.	2023	82.892	12.076	2.529	0.959	-0.898	20.793

💡 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	–	–	–	17	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0320	45.9	82.83	12.11	2.52	0.65	-0.56	25.87	0.48

💡 Note: The % column shows the percentage of members that CWWDL 14569 shares with each listed object.

Visualization

ℹ️