CWWDL 14300

0.00 UTI

0.5

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CA

Number of members (P>50%) 50

Radius (P>50% members) 8.5 [arcmin]

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 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 14300 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, below 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 14300 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	–	346.427	49.39	1.805	2.62	-1.932	-10.536
Chi et al.	2023	346.503	49.402	1.839	2.575	-1.844	-12.866

💡 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	–	–	–	5	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2275	100.0	346.45	49.38	1.8	2.63	-1.95	-11.11	0.0
UBC 171	100.0	346.41	49.38	1.79	2.64	-1.99	-11.02	0.08
UPK 185	100.0	346.41	49.38	1.79	2.64	-1.96	-11.02	0.86

💡 Note: The % column shows the percentage of members that CWWDL 14300 shares with each listed object.

Visualization

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