CWWDL 2624

0.04 UTI

0.0

C_N

0.28

C_dens

0.38

C_C3

0.0

C_lit

0.32

C_dup

C3 classification BC

Number of members (P>50%) 19

Radius (P>50% members) 5.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.28 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWWDL 2624 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a moderate 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 2624 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	–	40.346	60.761	0.414	-0.496	-0.295	-81.548
Chi et al.	2023	40.159	60.795	0.411	-0.474	-0.345	-61.947

💡 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	–	–	–	9	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 420	68.0	40.37	60.84	0.43	-0.65	-0.21	-61.21	0.47
CWWDL 10668	28.0	39.85	60.77	0.39	-0.56	-0.34	-41.75	0.03
CWWDL 10681	4.0	40.28	61.13	0.41	-0.28	-0.27	–	0.05

💡 Note: The % column shows the percentage of members that CWWDL 2624 shares with each listed object.

Visualization

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