CWWDL 14172

0.03 UTI

0.32

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.09

C_dup

C3 classification CB

Number of members (P>50%) 32

Radius (P>50% members) 4.4 [arcmin]

C_N 0.32 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.09 Very likely duplicate

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

Overview

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CWWDL 14172 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 14172 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	–	348.884	59.997	0.69	-1.751	-1.358	-14.477
Chi et al.	2023	348.897	60.012	0.692	-1.693	-1.309	–

💡 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	–	–	–	76	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0203	90.6	348.86	59.99	0.7	-1.75	-1.37	-6.56	0.47

💡 Note: The % column shows the percentage of members that CWWDL 14172 shares with each listed object.

Visualization

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