CWNU 2944

0.09 UTI

0.48

C_N

0.17

C_dens

0.25

C_C3

0.0

C_lit

0.48

C_dup

C3 classification DB

Number of members (P>50%) 48

Radius (P>50% members) 3.8 [arcmin]

C_N 0.48 Poorly populated
C_dens 0.17 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.48 Possibly duplicate

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

Overview

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CWNU 2944 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large distance, below 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 2944 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	–	122.157	-36.228	0.148	-1.787	2.995	–
He et al.	2023	122.166	-36.236	0.14	-1.789	2.999	–

💡 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	2.50	–	398	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2034	52.1	122.15	-36.23	0.15	-1.78	2.98	–	0.19

💡 Note: The % column shows the percentage of members that CWNU 2944 shares with each listed object.

Visualization

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