CWWDL 13969

0.00 UTI

0.4

C_N

0.7

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 40

Stellar density (N₅₀/rad) 3.5 [N/pc²]

C3 classification AB

C_N 0.4 Poorly populated
C_dens 0.7 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CWWDL 13969 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a near-solar metallicity, young 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, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13969 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	146.87	-50.541	0.644	-7.154	5.026	20.918
Chi et al.	2023	146.887	-50.553	0.646	-7.174	5.076	19.516

💡 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–	–	–	–	25	0.370	–	–	–
Chi et al.	2023	–	–	–	25	0.370	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 184	100.0	146.87	-50.56	0.64	-7.14	5.01	13.24	0.0
Theia 6111	100.0	146.9	-50.57	0.64	-7.15	5.0	18.59	0.0
UBC 1465	100.0	146.89	-50.57	0.64	-7.15	5.0	20.53	0.49
CWWDL 14184	97.5	146.87	-50.55	0.65	-7.14	5.01	18.79	0.0

💡 Note: The % column shows the percentage of members that CWWDL 13969 shares with each listed object.

Visualization

ℹ️