CWWDL 10960

0.06 UTI

0.27

C_N

0.17

C_dens

0.5

C_C3

0.0

C_lit

0.33

C_dup

C3 classification BB

Number of members (P>50%) 27

Radius (P>50% members) 5.1 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.17 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.33 Possibly duplicate

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

Overview

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CWWDL 10960 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, very 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 Very young

Data

🔍 Search references for CWWDL 10960 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	–	115.428	-17.501	0.261	-1.956	2.454	–
Chi et al.	2023	115.451	-17.368	0.265	-1.978	2.446	71.852

💡 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	–	–	–	10	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 455	66.7	115.39	-17.58	0.27	-1.96	2.45	89.22	0.65

💡 Note: The % column shows the percentage of members that CWWDL 10960 shares with each listed object.

Visualization

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