CWWDL 14179

0.03 UTI

0.3

C_N

0.29

C_dens

0.38

C_C3

0.0

C_lit

0.17

C_dup

C3 classification CB

Number of members (P>50%) 30

Radius (P>50% members) 10.5 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.29 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

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

Overview

ℹ️

CWWDL 14179 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 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 Young

Data

🔍 Search references for CWWDL 14179 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	115.541	-21.874	0.676	-2.506	1.714	39.804
Chi et al.	2023	115.59	-21.994	0.674	-2.503	1.701	36.321

💡 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	–	–	–	71	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 43	83.3	115.48	-21.85	0.67	-2.5	1.69	40.05	0.27
Theia 3524	76.7	115.55	-21.98	0.68	-2.5	1.72	34.46	0.05

💡 Note: The % column shows the percentage of members that CWWDL 14179 shares with each listed object.

Visualization

ℹ️