CWNU 4796

0.05 UTI

0.28

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.14

C_dup

C3 classification CB

Number of members (P>50%) 28

Radius (P>50% members) 0.9 [arcmin]

C_N 0.28 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.14 Likely duplicate

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

Overview

ℹ️

CWNU 4796 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant High extinction Very young

Data

🔍 Search references for CWNU 4796 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	84.693	30.498	0.209	-0.238	-1.699	–
He et al.	2023	84.694	30.498	0.216	-0.215	-1.723	–

💡 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	6.03	4.45	–	3	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Gaia 7	85.7	84.69	30.5	0.22	-0.25	-1.67	–	0.34

💡 Note: The % column shows the percentage of members that CWNU 4796 shares with each listed object.

Visualization

ℹ️