CWNU 108

0.21 UTI

0.55

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.55

C_dup

C3 classification BC

Number of members (P>50%) 60

Radius (P>50% members) 7.7 [arcmin]

C_N 0.55 Moderately populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.55 Likely unique

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

Overview

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CWNU 108 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is rarely studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Metal-rich Young

Data

🔍 Search references for CWNU 108 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	354.562	57.762	0.714	-4.611	-1.778	-21.387
He et al.	2022	354.512	57.752	0.71	-4.59	-1.77	–

💡 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	1.70	1.68	–	50	0.862	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0207	45.0	354.47	57.78	0.72	-4.6	-1.8	-13.03	0.5

💡 Note: The % column shows the percentage of members that CWNU 108 shares with each listed object.

Visualization

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