CWWDL 13965

0.14 UTI

0.43

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.33

C_dup

C3 classification AB

Number of members (P>50%) 43

Radius (P>50% members) 5.2 [arcmin]

C_N 0.43 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High 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 13965 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a metal-poor, 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.

Metal-poor Very young

Data

🔍 Search references for CWWDL 13965 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	–	138.978	-44.849	0.554	-5.194	5.14	20.178
Chi et al.	2023	138.891	-44.83	0.542	-5.093	5.031	20.178

💡 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	–	–	–	2	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 535	67.4	138.99	-44.86	0.56	-5.2	5.15	20.18	0.0
Theia 3337	67.4	138.99	-44.87	0.56	-5.2	5.15	20.18	0.03
UBC 1586	67.4	138.99	-44.86	0.56	-5.2	5.15	20.18	0.36

💡 Note: The % column shows the percentage of members that CWWDL 13965 shares with each listed object.

Visualization

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