CWWDL 2661

0.10 UTI

0.77

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.2

C_dup

C3 classification AB

Number of members (P>50%) 152

Radius (P>50% members) 4.6 [arcmin]

C_N 0.77 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWWDL 2661 is a rich, very dense object of 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 2661 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	–	97.786	15.072	0.309	-0.168	-1.069	46.559
Chi et al.	2023	97.782	15.088	0.299	-0.147	-1.062	43.057

💡 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	–	–	–	107	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 203	80.3	97.79	15.06	0.31	-0.16	-1.08	45.03	0.7
OC 0326	38.2	97.79	15.06	0.32	-0.17	-1.09	43.8	0.0
CWWDL 10879	0.7	97.21	15.19	0.24	0.03	-1.25	56.51	0.08

💡 Note: The % column shows the percentage of members that CWWDL 2661 shares with each listed object.

Visualization

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