CWWDL 14686

0.00 UTI

0.0

C_N

0.34

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BB

Number of members (P>50%) 23

Radius (P>50% members) 45.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.34 Loose
C_C3 0.5 Intermediate 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 14686 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane. It is catalogued as a near-solar metallicity, 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14686 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	–	102.715	-6.298	3.608	-7.13	-2.367	23.599
Chi et al.	2023	102.288	-6.222	3.654	-7.078	-2.358	10.107

💡 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	–	–	–	1	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2439	100.0	103.56	-5.88	3.5	-7.36	-2.45	20.16	0.58
OCSN 211	84.0	103.61	-5.94	3.49	-7.37	-2.43	20.37	0.0
ZHBJZ 1	48.0	103.74	-5.89	3.49	-7.41	-2.44	20.51	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14686 shares with each listed object.

Visualization

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