NGC 2932

(MWSC 1694; ESO 261 10)

0.16 UTI

0.0

C_N

0.05

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 15

Radius (P>50% members) 7.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.25 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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NGC 2932 is a sparse, very loose object of 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 is poorly studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Intermediate age

Dias et al. (2002)
Asterism (Archinal, B. A. & Hynes, S. J. 2003)

Data

🔍 Search references for NGC 2932 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	–	143.906	-46.846	0.267	-5.017	3.109	104.12
Just et al.	2023	143.862	-46.806	–	–	–	–
Bica et al.	2019	143.855	-46.823	–	–	–	–
Kharchenko et al.	2016	143.862	-46.806	–	–	–	–
Kharchenko et al.	2013	143.866	-46.81	–	-2.71	7.11	–

💡 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
Just et al.	2023	–	–	–	708	–	640	–	–
Kharchenko et al.	2016	2.92	1.68	–	708	–	–	–	–
Kharchenko et al.	2013	2.92	1.68	–	708	–	–	–	–

Visualization

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