CWNU 1068

0.02 UTI

0.25

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.04

C_dup

C3 classification AB

Number of members (P>50%) 25

Radius (P>50% members) 4.7 [arcmin]

C_N 0.25 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

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

Overview

ℹ️

CWNU 1068 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively 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.

⚠️ 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.

Low extinction Very young

Data

🔍 Search references for CWNU 1068 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	74.87	37.974	0.909	-0.567	-2.86	-0.746
He et al.	2022	74.908	37.965	0.937	-0.532	-2.912	–

💡 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	–	0.10	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0744	96.0	74.87	37.97	0.9	-0.56	-2.88	-11.66	0.66

💡 Note: The % column shows the percentage of members that CWNU 1068 shares with each listed object.

Visualization

ℹ️