CWWDL 2957

0.04 UTI

0.0

C_N

0.53

C_dens

0.75

C_C3

0.0

C_lit

0.16

C_dup

C3 classification AB

Number of members (P>50%) 23

Radius (P>50% members) 2.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.53 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWWDL 2957 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a metal-poor, 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. See table with shared members information.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 2957 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	–	92.084	28.073	0.258	-0.16	-1.691	4.423
Chi et al.	2023	92.076	28.058	0.268	-0.034	-1.651	13.116

💡 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	–	–	–	123	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1295	84.0	92.08	28.07	0.26	-0.2	-1.69	0.53	0.27
LISC 2967	84.0	92.08	28.07	0.25	-0.18	-1.67	4.42	0.36

💡 Note: The % column shows the percentage of members that CWWDL 2957 shares with each listed object.

Visualization

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