CWWDL 11962

0.01 UTI

0.0

C_N

0.02

C_dens

0.12

C_C3

0.0

C_lit

0.44

C_dup

C3 classification DC

Number of members (P>50%) 16

Radius (P>50% members) 11.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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CWWDL 11962 is a sparse, very loose object of very low 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 possibly a duplicate object, which shares a significant 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 11962 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	–	90.803	28.411	0.266	0.384	-1.388	51.695
Chi et al.	2023	90.823	28.436	0.266	0.367	-1.357	2.689

💡 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	–	–	–	186	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 1377	56.0	90.79	28.46	0.26	0.4	-1.45	14.83	0.03
FoF 1372	4.0	90.55	28.87	0.27	0.26	-1.48	5.04	0.03
FoF 1375	4.0	91.04	28.05	0.22	0.39	-1.09	33.92	0.37

💡 Note: The % column shows the percentage of members that CWWDL 11962 shares with each listed object.

Visualization

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