CWNU 2941

0.15 UTI

0.52

C_N

0.76

C_dens

0.12

C_C3

0.0

C_lit

0.53

C_dup

C3 classification DC

Number of members (P>50%) 55

Radius (P>50% members) 4.2 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.76 Dense
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.53 Likely unique

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

Overview

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CWNU 2941 is a moderately populated, dense object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 2941 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	–	86.223	35.481	0.321	1.438	-2.903	-2.204
He et al.	2023	86.219	35.486	0.313	1.438	-2.903	-2.2

💡 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	2.82	2.65	–	398	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1362	47.3	86.24	35.49	0.32	1.39	-2.91	-2.2	0.29

💡 Note: The % column shows the percentage of members that CWNU 2941 shares with each listed object.

Visualization

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