VVV 100

(VVV-CL 100)

0.43 UTI

0.39

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BA

Number of members (P>50%) 39

Radius (P>50% members) 2.7 [arcmin]

C_N 0.39 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High 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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VVV 100 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 15 years.

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

No fundamental parameters

Data

🔍 Search references for VVV 100 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	–	259.832	-39.061	0.58	0.988	-1.135	–
Borissova et al.	2011	259.812	-39.076	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 4	100.0	259.85	-39.07	0.59	0.99	-1.14	–	0.15
CWWDL 13634	100.0	259.84	-39.06	0.59	0.99	-1.13	–	0.03
OC 0681	100.0	259.83	-39.06	0.58	0.99	-1.13	–	0.05

💡 Note: The % column shows the percentage of members that VVV 100 shares with each listed object.

Visualization

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