CWWDL 2237

0.22 UTI

0.77

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.39

C_dup

C3 classification AA

Number of members (P>50%) 157

Radius (P>50% members) 3.6 [arcmin]

C_N 0.77 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.39 Possibly duplicate

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

Overview

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CWWDL 2237 is a rich, very dense object of very high 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 2237 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	–	182.341	-61.326	0.335	-6.906	0.6	-41.263
Chi et al.	2023	182.325	-61.326	0.338	-6.874	0.623	-26.157

💡 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	–	–	–	132	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch J1209.3-6120	72.6	182.34	-61.32	0.34	-6.92	0.59	-41.86	0.01
UBC 1514	61.1	182.34	-61.32	0.33	-6.92	0.58	-42.3	0.55

💡 Note: The % column shows the percentage of members that CWWDL 2237 shares with each listed object.

Visualization

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