CWWDL 2763

0.10 UTI

0.26

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.23

C_dup

C3 classification AA

Number of members (P>50%) 26

Radius (P>50% members) 2.3 [arcmin]

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

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

Overview

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CWWDL 2763 is a poorly 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 metal-poor, young 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. See table with shared members information.

Metal-poor Young

Data

🔍 Search references for CWWDL 2763 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	–	175.404	-59.572	0.415	-7.251	1.216	-27.768
Chi et al.	2023	175.407	-59.551	0.42	-7.171	1.176	-32.566

💡 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	–	–	–	27	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1504	76.9	175.39	-59.57	0.42	-7.27	1.22	-27.77	0.45

💡 Note: The % column shows the percentage of members that CWWDL 2763 shares with each listed object.

Visualization

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