CWWDL 14426

0.00 UTI

0.37

C_N

0.67

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 37

Radius (P>50% members) 10.0 [arcmin]

C3 classification AB

C_N 0.37 Poorly populated
C_dens 0.67 Moderately 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 14426 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close 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 14426 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–	218.02	-58.746	0.876	-1.223	-3.041	8.435
Chi et al.	2023	218.098	-58.748	0.887	-1.193	-3.011	2.911

💡 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–	–	–	–	41	-0.880	–	–	–
Chi et al.	2023	–	–	–	41	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 13	100.0	218.1	-58.71	0.88	-1.22	-3.08	4.96	0.59

💡 Note: The % column shows the percentage of members that CWWDL 14426 shares with each listed object.

Visualization

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