CWWDL 14045

0.00 UTI

0.52

C_N

0.9

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 54

Stellar density (N₅₀/rad) 4.5 [N/pc²]

C3 classification AA

C_N 0.52 Moderately populated
C_dens 0.9 Very dense
C_C3 1.0 Very 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 14045 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a near-solar metallicity, 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 moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14045 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	191.785	-59.386	0.612	-5.958	-0.225	-23.548
Chi et al.	2023	191.869	-59.395	0.622	-5.977	-0.22	-11.907

💡 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–	–	–	–	8	0.070	–	–	–
Chi et al.	2023	–	–	–	8	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 290	100.0	191.89	-59.37	0.61	-5.93	-0.25	-23.5	0.76
CWWDL 14223	42.6	191.94	-59.37	0.63	-5.93	-0.28	-19.79	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14045 shares with each listed object.

Visualization

ℹ️