CWNU 3247

0.08 UTI

0.5

C_N

0.86

C_dens

0.25

C_C3

0.0

C_lit

0.24

C_dup

C3 classification DB

Number of members (P>50%) 51

Radius (P>50% members) 2.4 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.86 Dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWNU 3247 is a moderately populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, near 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 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 3247 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	–	100.833	2.373	0.202	-0.145	0.742	77.162
He et al.	2023	100.83	2.375	0.198	-0.119	0.742	–

💡 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	4.47	2.95	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1654	76.5	100.83	2.38	0.2	-0.15	0.72	77.16	0.27

💡 Note: The % column shows the percentage of members that CWNU 3247 shares with each listed object.

Visualization

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