CWNU 2951

0.34 UTI

0.35

C_N

0.86

C_dens

0.5

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 35

Radius (P>50% members) 1.7 [arcmin]

C_N 0.35 Poorly populated
C_dens 0.86 Dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 2951 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.78 kpc) differs significantly from the median photometric distance (~4.07 kpc).

Distant Moderate extinction Old

Data

🔍 Search references for CWNU 2951 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	–	133.534	-49.643	0.173	-2.513	2.878	–
He et al.	2023	133.539	-49.643	0.177	-2.502	2.878	–

💡 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	4.07	2.55	–	2512	–	–	–	–

Visualization

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