CWWDL 14542

0.00 UTI

0.54

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BA

Number of members (P>50%) 57

Radius (P>50% members) 13.0 [arcmin]

C_N 0.54 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 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14542 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Very close Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 14542 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	–	301.231	-10.533	2.273	1.467	-7.931	-16.391
Wei et al.	2025	301.25	-10.533	2.279	1.523	-7.841	–
Chi et al.	2023	301.232	-10.546	2.256	1.41	-7.891	-18.192

💡 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
Wei et al.	2025	0.45	0.68	–	1120	-0.250	157	0.39	–
Chi et al.	2023	–	–	–	5	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Alessi 10	100.0	301.25	-10.55	2.26	1.48	-7.88	-15.44	0.96

💡 Note: The % column shows the percentage of members that CWWDL 14542 shares with each listed object.

Visualization

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