CWWDL 633

0.04 UTI

0.34

C_N

0.79

C_dens

0.75

C_C3

0.0

C_lit

0.12

C_dup

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 3.6 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.79 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

ℹ️

CWWDL 633 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 633 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	110.183	-17.874	0.357	-1.018	1.343	–
Chi et al.	2023	110.183	-17.885	0.361	-1.175	1.292	37.768

💡 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	–	–	–	38	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1372	88.2	110.18	-17.88	0.35	-1.01	1.35	46.98	0.54
CWNU 374	79.4	110.18	-17.88	0.36	-1.01	1.35	46.98	0.04

💡 Note: The % column shows the percentage of members that CWWDL 633 shares with each listed object.

Visualization

ℹ️