CWNU 2968

0.02 UTI

0.51

C_N

0.31

C_dens

0.75

C_C3

0.0

C_lit

0.06

C_dup

C3 classification AB

Number of members (P>50%) 52

Radius (P>50% members) 2.5 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.31 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

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

Overview

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CWNU 2968 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a large^* distance, well below 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.

(*): The parallax distance estimate (~8.03 kpc) differs significantly from the median photometric distance (~6.03 kpc).

Very distant Low extinction Intermediate age

Data

🔍 Search references for CWNU 2968 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	–	104.278	-23.565	0.125	-0.42	2.001	72.602
He et al.	2023	104.281	-23.568	0.139	-0.421	2.001	72.6

💡 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	6.03	0.35	–	631	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1860	94.2	104.28	-23.57	0.13	-0.42	2.0	72.6	0.41

💡 Note: The % column shows the percentage of members that CWNU 2968 shares with each listed object.

Visualization

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