CWNU 3026

0.01 UTI

0.37

C_N

0.41

C_dens

0.38

C_C3

0.0

C_lit

0.05

C_dup

C3 classification BC

Number of members (P>50%) 37

Radius (P>50% members) 11.6 [arcmin]

C_N 0.37 Poorly populated
C_dens 0.41 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

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

Overview

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CWNU 3026 is a poorly populated, loose object of low 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 very 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 3026 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	–	106.05	-0.057	0.799	-0.073	-1.82	-5.586
He et al.	2023	106.05	-0.054	0.785	-0.073	-1.812	-5.59

💡 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	1.35	1.00	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1691	94.6	106.05	-0.01	0.8	-0.07	-1.83	1.31	0.33

💡 Note: The % column shows the percentage of members that CWNU 3026 shares with each listed object.

Visualization

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