CWWDL 14543

0.12 UTI

0.54

C_N

0.94

C_dens

1.0

C_C3

0.0

C_lit

0.24

C_dup

C3 classification AA

Number of members (P>50%) 58

Radius (P>50% members) 24.2 [arcmin]

C_N 0.54 Moderately populated
C_dens 0.94 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWWDL 14543 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.

⚠️ Warning: This is 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 14543 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	–	339.723	37.293	2.008	-1.547	-6.123	-13.973
Chi et al.	2023	339.877	37.168	2.022	-1.585	-6.037	-9.556

💡 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	–	–	–	3	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 39	75.9	339.22	37.76	2.04	-1.76	-6.04	-13.08	0.84
OCSN 29	55.2	339.15	37.72	2.03	-1.72	-6.19	-13.08	0.02
FoF 2379	17.2	339.63	38.15	1.98	-1.56	-5.8	-21.27	0.16

💡 Note: The % column shows the percentage of members that CWWDL 14543 shares with each listed object.

Visualization

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