CWNU 3059

0.38 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.76

C_dup

N₅₀ (P>50% members) 104

Stellar density (N₅₀/rad) 6.0 [N/pc²]

C3 classification AB

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.76 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3059 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Intermediate age

Data

🔍 Search references for CWNU 3059 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	99999–	68.822	47.295	0.174	0.483	-0.852	-44.762
He et al.	2023	68.825	47.291	0.168	0.475	-0.845	-41.52

💡 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]	B_frac	BSS
UCC	99999–	4.9	4.1	–	200	–	–	–	–
He et al.	2023	4.90	4.10	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1242	24.0	68.81	47.29	0.17	0.49	-0.85	–	0.4

💡 Note: The % column shows the percentage of members that CWNU 3059 shares with each listed object.

Visualization

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