CWWDL 14210

0.13 UTI

0.57

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.28

C_dup

C3 classification AB

Number of members (P>50%) 64

Radius (P>50% members) 7.2 [arcmin]

C_N 0.57 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

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CWWDL 14210 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 14210 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	–	330.466	56.046	0.641	-1.976	-1.698	34.448
Chi et al.	2023	330.493	56.074	0.659	-1.889	-1.777	-14.965

💡 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	–	–	–	20	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 28	71.9	330.47	56.03	0.64	-2.01	-1.66	34.45	0.51
UBC 1154	71.9	330.47	56.04	0.64	-2.0	-1.67	34.45	0.01
CWWDL 13945	57.8	330.47	56.03	0.64	-2.0	-1.67	34.45	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14210 shares with each listed object.

Visualization

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