CWWDL 8942

0.00 UTI

0.36

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 36

Stellar density (N₅₀/rad) 18.0 [N/pc²]

C3 classification BB

C_N 0.36 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate 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 8942 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate 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 very 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 8942 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	123.894	-33.904	0.494	-2.908	2.905	31.767
Chi et al.	2023	123.906	-33.928	0.489	-2.908	2.87	40.059

💡 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–	–	–	–	76	-0.100	–	–	–
Chi et al.	2023	–	–	–	76	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 475	100.0	123.89	-33.89	0.48	-2.9	2.9	31.77	0.59

💡 Note: The % column shows the percentage of members that CWWDL 8942 shares with each listed object.

Visualization

ℹ️