CWNU 4776

0.08 UTI

0.0

C_N

0.35

C_dens

0.25

C_C3

0.0

C_lit

0.68

C_dup

C3 classification DB

Number of members (P>50%) 24

Radius (P>50% members) 3.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.35 Loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.68 Likely unique

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

Overview

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CWNU 4776 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported 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.

Distant Low extinction Very young

Data

🔍 Search references for CWNU 4776 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	–	209.236	-63.003	0.297	-6.626	-2.437	-52.699
He et al.	2023	209.283	-63.006	0.301	-6.626	-2.438	–

💡 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.	2023	3.09	0.10	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2651	32.0	209.29	-63.02	0.29	-6.44	-2.41	-46.58	0.15

💡 Note: The % column shows the percentage of members that CWNU 4776 shares with each listed object.

Visualization

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