CWNU 4494

0.03 UTI

0.41

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.07

C_dup

C3 classification AC

Number of members (P>50%) 41

Radius (P>50% members) 1.7 [arcmin]

C_N 0.41 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.07 Very likely duplicate

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

Overview

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CWNU 4494 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported 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.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 4494 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	–	67.677	54.047	0.213	-0.25	-0.052	-42.059
He et al.	2023	67.742	54.014	0.187	-0.229	-0.116	-47.99

💡 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	4.37	2.05	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Juchert J0430.6+5402	92.7	67.67	54.05	0.2	-0.22	-0.04	-39.38	0.4

💡 Note: The % column shows the percentage of members that CWNU 4494 shares with each listed object.

Visualization

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