VVVX CL032

0.06 UTI

0.0

C_N

0.05

C_dens

0.25

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 11

Stellar density (N₅₀/rad) 0.2 [N/pc²]

C3 classification DB

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

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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VVVX CL032 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~3.17 kpc) differs significantly from the median photometric distance (~2.31 kpc).

⚠️ 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

Borissova et al. (2018)
B9 star + group of stars.

Data

🔍 Search references for VVVX CL032 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	99999–	239.752	-56.23	0.316	-4.344	-4.227	8.215
Borissova et al.	2018	239.836	-56.233	0.319	-4.358	-4.217	-38.27

💡 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]	B_frac	BSS
UCC	99999–	2.31	–	–	–	–	–	–	–
Borissova et al.	2018	2.31	–	–	–	–	–	–	–

Visualization

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