CWWDL 14076

0.00 UTI

0.47

C_N

0.56

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 47

Stellar density (N₅₀/rad) 2.8 [N/pc²]

C3 classification AB

C_N 0.47 Poorly populated
C_dens 0.56 Moderately dense
C_C3 0.75 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 14076 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, 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 Young

Data

🔍 Search references for CWWDL 14076 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–	106.838	4.27	0.482	-0.353	-1.656	29.559
Chi et al.	2023	106.84	4.276	0.49	-0.347	-1.626	33.053

💡 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–	–	–	–	50	-0.580	–	–	–
Chi et al.	2023	–	–	–	50	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1337	100.0	106.84	4.26	0.48	-0.35	-1.66	29.56	0.05
HXHWL 60	95.7	106.83	4.26	0.48	-0.36	-1.66	29.56	0.49

💡 Note: The % column shows the percentage of members that CWWDL 14076 shares with each listed object.

Visualization

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