CWNU 63

0.03 UTI

0.6

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.06

C_dup

C3 classification AB

Number of members (P>50%) 70

Radius (P>50% members) 4.8 [arcmin]

C_N 0.6 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

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

Overview

ℹ️

CWNU 63 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied 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.

Relatively close Moderate extinction Metal-rich Intermediate age

Data

🔍 Search references for CWNU 63 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	283.469	-4.649	0.427	-0.639	-1.12	20.259
He et al.	2022	283.458	-4.638	0.43	-0.65	-1.12	26.7

💡 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
He et al.	2022	2.00	2.28	–	126	0.744	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1044	94.3	283.47	-4.64	0.43	-0.64	-1.12	20.26	0.62
CWWDL 13354	45.7	283.47	-4.65	0.43	-0.65	-1.12	20.26	0.0

💡 Note: The % column shows the percentage of members that CWNU 63 shares with each listed object.

Visualization

ℹ️