CWNU 1040

0.50 UTI

0.49

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 49

Stellar density (N₅₀/rad) 43.6 [N/pc²]

C3 classification AA

C_N 0.49 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

CWNU 1040 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Moderate extinction Very young

Data

🔍 Search references for CWNU 1040 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	10.841	61.962	1.837	3.359	-2.2	-9.524
He et al.	2022	10.838	61.944	1.838	3.352	-2.159	–

💡 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]	B_frac	BSS
UCC	99999–	–	2.8	–	6	–	–	–	–
He et al.	2022	–	2.80	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 6	100.0	10.84	61.97	1.83	3.39	-2.19	-9.52	0.03

💡 Note: The % column shows the percentage of members that CWNU 1040 shares with each listed object.

Visualization

ℹ️