CWWDL 13960

0.01 UTI

0.5

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.02

C_dup

N₅₀ (P>50% members) 51

Stellar density (N₅₀/rad) 13.6 [N/pc²]

C3 classification CC

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

CWWDL 13960 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 13960 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	105.952	0.262	0.466	-1.326	1.04	14.601
Chi et al.	2023	105.96	0.24	0.473	-1.289	1.071	33.176

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	123	-0.400	–	–	–
Chi et al.	2023	–	–	–	123	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 131	98.0	105.95	0.26	0.47	-1.33	1.04	14.6	0.05
UBC 1342	92.2	105.95	0.26	0.47	-1.33	1.02	–	0.5

💡 Note: The % column shows the percentage of members that CWWDL 13960 shares with each listed object.

Visualization

ℹ️