VVV 164

(VVV-CL 164; MGC 5; MGC Pis 24W)

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0.00 UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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VVV 164 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 7 years.

âš ī¸ 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.

No fundamental parameters

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 261.174 -34.201 0.548 -0.875 -1.98 8.637
Bica et al. 2019 261.13 -34.216 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 6357 100.0 261.2 -34.21 0.55 -0.85 -2.1 6.35 0.79
OC 0688 30.2 261.29 -34.35 0.55 -0.91 -2.15 18.21 0.05

💡 Note: The % column shows the percentage of members that VVV 164 shares with each listed object.

Visualization

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