CWWDL 14484

0.01 UTI

0.51

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.02

C_dup

C3 classification CA

Number of members (P>50%) 52

Radius (P>50% members) 9.3 [arcmin]

C_N 0.51 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

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

Overview

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CWWDL 14484 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, above 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 14484 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	–	352.307	66.93	1.271	-1.371	-0.129	-16.761
Chi et al.	2023	352.312	66.946	1.269	-1.359	-0.081	-9.75

💡 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	–	–	–	6	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 224	98.1	352.26	66.94	1.27	-1.37	-0.16	-16.76	0.55
UBC 1187	50.0	352.22	66.93	1.27	-1.36	-0.16	-12.88	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14484 shares with each listed object.

Visualization

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