CWWDL 13543

0.01 UTI

0.35

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.03

C_dup

C3 classification BC

Number of members (P>50%) 35

Radius (P>50% members) 1.8 [arcmin]

C_N 0.35 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

ℹ️

CWWDL 13543 is a poorly populated, very dense object of low 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.

⚠️ 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 13543 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	116.552	-26.206	0.472	-3.686	3.076	25.661
Chi et al.	2023	116.562	-26.2	0.479	-3.721	3.064	25.661

💡 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	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 463	97.1	116.55	-26.21	0.47	-3.69	3.08	25.66	0.57

💡 Note: The % column shows the percentage of members that CWWDL 13543 shares with each listed object.

Visualization

ℹ️