CWWDL 14621

0.00 UTI

0.45

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BA

Number of members (P>50%) 45

Radius (P>50% members) 20.5 [arcmin]

C_N 0.45 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High 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 14621 is a poorly populated, very dense object of high 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, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14621 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	–	323.028	48.297	3.384	-7.601	-19.901	-6.534
Chi et al.	2023	323.283	48.179	3.381	-7.603	-19.92	-6.352

💡 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	–	–	–	6	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Melotte 236	100.0	322.8	48.25	3.36	-7.45	-19.73	-5.94	0.97
Theia 517	100.0	322.8	48.25	3.36	-7.45	-19.74	-6.07	0.07
CWWDL 14690	80.0	322.87	48.25	3.4	-7.49	-19.96	-6.46	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14621 shares with each listed object.

Visualization

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