CWWDL 2764

0.15 UTI

0.58

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.3

C_dup

C3 classification AA

Number of members (P>50%) 67

Radius (P>50% members) 2.8 [arcmin]

C_N 0.58 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.3 Possibly duplicate

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

Overview

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CWWDL 2764 is a moderately populated, 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, 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. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 2764 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	–	180.166	-60.498	0.307	-6.361	0.697	2.307
Chi et al.	2023	180.143	-60.497	0.293	-6.41	0.73	-14.675

💡 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	–	–	–	54	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 282	70.1	180.18	-60.5	0.31	-6.34	0.67	56.84	0.65
OC 0576	37.3	180.17	-60.5	0.3	-6.36	0.68	–	0.0

💡 Note: The % column shows the percentage of members that CWWDL 2764 shares with each listed object.

Visualization

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