CWWDL 14343

0.01 UTI

0.3

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AB

Number of members (P>50%) 30

Radius (P>50% members) 4.4 [arcmin]

C_N 0.3 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

ℹ️

CWWDL 14343 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 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.

Metal-poor Very young

Data

🔍 Search references for CWWDL 14343 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	107.359	-12.038	0.854	-3.281	0.961	21.103
Chi et al.	2023	107.323	-12.037	0.884	-3.307	0.994	49.956

💡 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	–	–	–	1	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CMa08	96.7	107.43	-12.28	0.86	-3.15	0.88	26.44	0.5
CWWDL 14345	76.7	107.43	-12.14	0.87	-3.2	0.92	22.81	0.01
OC 0377	73.3	107.42	-12.04	0.85	-3.26	0.94	20.73	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14343 shares with each listed object.

Visualization

ℹ️