CWNU 4703

0.02 UTI

0.25

C_N

0.06

C_dens

0.25

C_C3

0.0

C_lit

0.16

C_dup

C3 classification CC

Number of members (P>50%) 25

Radius (P>50% members) 3.9 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.06 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWNU 4703 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age 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.

(*): The parallax distance estimate (~7.84 kpc) differs significantly from the median photometric distance (~5.13 kpc).

Very distant High extinction Intermediate age

Data

🔍 Search references for CWNU 4703 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	–	332.698	57.213	0.128	-2.484	-1.919	-119.281
He et al.	2023	332.701	57.212	0.134	-2.504	-1.911	-119.28

💡 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	5.13	3.60	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 792	84.0	332.7	57.24	0.13	-2.52	-1.91	-119.28	0.15

💡 Note: The % column shows the percentage of members that CWNU 4703 shares with each listed object.

Visualization

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