CWWDL 14090

0.00 UTI

1.0

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 996

Stellar density (N₅₀/rad) 95.4 [N/pc²]

C3 classification AA

C_N 1.0 Very rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 14090 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a 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 14090 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–	132.845	11.817	1.152	-10.976	-2.912	33.786
Chi et al.	2023	132.849	11.827	1.15	-10.96	-2.912	33.866

💡 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–	–	–	–	19	-0.880	–	–	–
Chi et al.	2023	–	–	–	19	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Melotte 94	100.0	132.85	11.82	1.15	-10.97	-2.91	33.91	1.0
Chupina 1	2.6	132.62	11.9	1.16	-10.99	-2.99	34.59	0.48
Chupina 3	2.5	132.85	11.41	1.15	-11.04	-2.83	34.39	0.45
Chupina 5	2.5	133.19	11.87	1.15	-10.96	-2.87	34.33	0.43
Chupina 2	1.9	132.64	12.26	1.14	-11.01	-2.96	33.83	0.4
Chupina 4	1.0	133.01	12.34	1.15	-10.93	-2.95	33.99	0.35
NGC 2678	0.9	132.58	11.36	1.05	-10.92	-2.82	35.48	0.28

💡 Note: The % column shows the percentage of members that CWWDL 14090 shares with each listed object.

Visualization

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