CWWDL 14250

0.14 UTI

0.49

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.29

C_dup

C3 classification AA

Number of members (P>50%) 49

Radius (P>50% members) 11.2 [arcmin]

C_N 0.49 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.29 Possibly duplicate

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

Overview

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CWWDL 14250 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14250 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	–	135.775	-34.947	1.197	-10.539	6.3	24.728
Chi et al.	2023	135.801	-34.974	1.201	-10.575	6.28	23.192

💡 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	–	–	–	25	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 508	71.4	135.77	-34.94	1.19	-10.54	6.3	24.11	0.77
UBC 477	51.0	135.77	-34.95	1.19	-10.54	6.32	24.45	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14250 shares with each listed object.

Visualization

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