CWNU 4709

0.03 UTI

0.0

C_N

0.14

C_dens

0.62

C_C3

0.0

C_lit

0.2

C_dup

C3 classification AC

Number of members (P>50%) 23

Radius (P>50% members) 18.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.14 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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CWNU 4709 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low 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.

Relatively close Low extinction Intermediate age

Data

🔍 Search references for CWNU 4709 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	–	127.912	-36.292	0.907	-5.018	4.563	21.052
He et al.	2023	127.9	-36.361	0.909	-5.051	4.565	20.5

💡 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	1.07	0.50	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2050	80.0	128.09	-36.34	0.91	-5.02	4.55	27.82	0.13

💡 Note: The % column shows the percentage of members that CWNU 4709 shares with each listed object.

Visualization

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