CWWDL 14652

0.00 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.01

C_dup

N₅₀ (P>50% members) 113

Stellar density (N₅₀/rad) 36.4 [N/pc²]

C3 classification AB

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.01 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14652 is a rich, very dense object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane. It is catalogued as a metal-poor, 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.

Metal-poor Very young

Data

🔍 Search references for CWWDL 14652 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	99999–	277.497	1.022	2.295	3.032	-8.828	-11.206
Chi et al.	2023	277.579	1.04	2.3	3.041	-8.752	4.978

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	1	-0.580	–	–	–
Chi et al.	2023	–	–	–	1	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 39	99.1	277.48	0.93	2.29	3.26	-8.73	-11.21	0.67

💡 Note: The % column shows the percentage of members that CWWDL 14652 shares with each listed object.

Visualization

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