CWWDL 14341

0.12 UTI

0.0

C_N

0.12

C_dens

0.62

C_C3

0.0

C_lit

0.8

C_dup

C3 classification AC

Number of members (P>50%) 16

Radius (P>50% members) 15.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.8 Very likely unique

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

Overview

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CWWDL 14341 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.8) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 14341 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	–	106.459	-11.125	0.855	-3.922	1.465	22.468
Chi et al.	2023	106.677	-11.203	0.901	-3.94	1.419	37.24

💡 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	–	–	–	107	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1178	20.0	106.34	-10.69	0.87	-3.72	1.62	25.06	0.66
VDB 92	8.0	106.05	-11.48	0.86	-4.41	1.56	24.52	0.95
FSR 1190	4.0	106.74	-11.32	0.85	-4.21	1.44	23.05	0.38

💡 Note: The % column shows the percentage of members that CWWDL 14341 shares with each listed object.

Visualization

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