CWWDL 2950

0.05 UTI

0.0

C_N

0.28

C_dens

0.25

C_C3

0.0

C_lit

0.44

C_dup

C3 classification CC

Number of members (P>50%) 16

Radius (P>50% members) 4.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.28 Loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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CWWDL 2950 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, intermediate-age 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 Intermediate age

Data

🔍 Search references for CWWDL 2950 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	–	71.769	49.047	0.344	0.867	-2.061	-26.731
Chi et al.	2023	71.742	49.071	0.351	0.793	-1.955	-15.267

💡 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	–	–	–	100	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 427	56.0	71.79	49.03	0.34	0.95	-2.26	-18.46	0.68

💡 Note: The % column shows the percentage of members that CWWDL 2950 shares with each listed object.

Visualization

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