CWNU 3063

0.15 UTI

0.46

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.3

C_dup

C3 classification AA

Number of members (P>50%) 46

Radius (P>50% members) 1.4 [arcmin]

C_N 0.46 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.3 Possibly duplicate

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

Overview

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CWNU 3063 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

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

(*): The parallax distance estimate (~5.42 kpc) differs significantly from the median photometric distance (~3.63 kpc).

Distant Moderate extinction Old

Data

🔍 Search references for CWNU 3063 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	–	44.858	64.273	0.184	0.235	0.332	-24.476
He et al.	2023	44.858	64.273	0.185	0.236	0.324	-24.48

💡 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	3.63	2.70	–	1585	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1109	69.6	44.85	64.27	0.18	0.24	0.31	-24.48	0.46

💡 Note: The % column shows the percentage of members that CWNU 3063 shares with each listed object.

Visualization

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