CWWDL 13588

0.12 UTI

0.0

C_N

0.05

C_dens

0.62

C_C3

0.0

C_lit

0.92

C_dup

C3 classification AC

Number of members (P>50%) 15

Radius (P>50% members) 12.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.92 Very likely unique

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

Overview

ℹ️

CWWDL 13588 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.92) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13588 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	174.313	-61.214	0.48	-6.453	0.97	–
Chi et al.	2023	174.37	-61.229	0.476	-6.454	0.967	-54.339

💡 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	–	–	–	44	-0.040	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 13832	8.0	174.44	-61.11	0.48	-6.5	1.09	12.46	0.14
NGC 3766	8.0	174.06	-61.61	0.48	-6.73	0.98	-18.96	1.0

💡 Note: The % column shows the percentage of members that CWWDL 13588 shares with each listed object.

Visualization

ℹ️