VVV 011

(VVV-CL 011)

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0.07 UTI
0.0
CN
0.0
Cdens
0.38
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.0 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

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VVV 011 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large distance, below 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.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

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 – 183.211 -62.71 0.032 -6.298 0.568 –
Bica et al. 2019 183.179 -62.709 – – – –
Borissova et al. 2011 183.171 -62.709 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3471 16.0 183.26 -62.71 0.17 -6.25 0.64 10.87 0.19
Alessi 52 12.0 183.14 -62.7 0.14 -6.36 0.69 – 0.16
CWNU 3697 4.0 182.98 -62.65 0.19 -6.36 0.67 – 0.06

💡 Note: The % column shows the percentage of members that VVV 011 shares with each listed object.

Visualization

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