CWNU 1108

0.30 UTI

0.25

C_N

0.5

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BA

Number of members (P>50%) 25

Radius (P>50% members) 88.8 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.5 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

ℹ️

CWNU 1108 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Low extinction Very young

Data

🔍 Search references for CWNU 1108 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	63.211	20.393	8.142	3.484	-13.84	15.044
He et al.	2022	63.089	20.107	8.088	3.409	-13.876	–

💡 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	–	0.15	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1340	100.0	68.02	19.84	8.24	0.7	-14.59	15.03	0.25
OCSN 118	100.0	62.83	20.3	8.24	3.7	-13.98	15.09	0.28
CWNU 1094	56.0	61.66	21.29	8.31	4.19	-14.51	15.0	0.44

💡 Note: The % column shows the percentage of members that CWNU 1108 shares with each listed object.

Visualization

ℹ️