CWNU 4778

0.08 UTI

0.0

C_N

0.15

C_dens

0.5

C_C3

0.0

C_lit

0.64

C_dup

C3 classification BB

Number of members (P>50%) 24

Radius (P>50% members) 31.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.15 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

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

Overview

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CWNU 4778 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a 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.

Close Moderate extinction Young

Data

🔍 Search references for CWNU 4778 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	–	24.141	67.218	1.607	-5.68	-0.495	-23.508
He et al.	2023	23.198	67.178	1.58	-5.68	-0.487	-24.31

💡 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	0.63	1.95	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 850	36.0	26.5	66.91	1.61	-5.6	-0.34	-19.94	0.16

💡 Note: The % column shows the percentage of members that CWNU 4778 shares with each listed object.

Visualization

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