VVV 006

(VVV-CL 006)

0.00 UTI

0.48

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 48

Stellar density (N₅₀/rad) 17.0 [N/pc²]

C3 classification AA

C_N 0.48 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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VVV 006 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity

Data

🔍 Search references for VVV 006 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–	177.314	-62.225	0.225	-7.744	1.321	-15.423
Donor et al.	2020	177.3	-62.208	–	-7.74	1.28	-14.1
Borissova et al.	2011	177.3	-62.208	–	–	–	–

💡 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–	–	–	–	–	0.160	–	–	–
Donor et al.	2020	–	–	–	–	0.160	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
SAI 116	100.0	177.32	-62.23	0.23	-7.74	1.35	-15.51	0.96
Teutsch 230	100.0	177.32	-62.23	0.23	-7.72	1.36	-15.47	0.03
OC 0572	66.7	177.31	-62.23	0.23	-7.74	1.36	-15.42	0.0

💡 Note: The % column shows the percentage of members that VVV 006 shares with each listed object.

Visualization

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